Philosophers
Mortimer Adler Rogers Albritton Alexander of Aphrodisias Samuel Alexander William Alston Anaximander G.E.M.Anscombe Anselm Louise Antony Thomas Aquinas Aristotle David Armstrong Harald Atmanspacher Robert Audi Augustine J.L.Austin A.J.Ayer Alexander Bain Mark Balaguer Jeffrey Barrett William Barrett William Belsham Henri Bergson George Berkeley Isaiah Berlin Richard J. Bernstein Bernard Berofsky Robert Bishop Max Black Susanne Bobzien Emil du BoisReymond Hilary Bok Laurence BonJour George Boole Émile Boutroux Daniel Boyd F.H.Bradley C.D.Broad Michael Burke Lawrence Cahoone C.A.Campbell Joseph Keim Campbell Rudolf Carnap Carneades Nancy Cartwright Gregg Caruso Ernst Cassirer David Chalmers Roderick Chisholm Chrysippus Cicero Randolph Clarke Samuel Clarke Anthony Collins Antonella Corradini Diodorus Cronus Jonathan Dancy Donald Davidson Mario De Caro Democritus Daniel Dennett Jacques Derrida René Descartes Richard Double Fred Dretske John Dupré John Earman Laura Waddell Ekstrom Epictetus Epicurus Austin Farrer Herbert Feigl Arthur Fine John Martin Fischer Frederic Fitch Owen Flanagan Luciano Floridi Philippa Foot Alfred Fouilleé Harry Frankfurt Richard L. Franklin Bas van Fraassen Michael Frede Gottlob Frege Peter Geach Edmund Gettier Carl Ginet Alvin Goldman Gorgias Nicholas St. John Green H.Paul Grice Ian Hacking Ishtiyaque Haji Stuart Hampshire W.F.R.Hardie Sam Harris William Hasker R.M.Hare Georg W.F. Hegel Martin Heidegger Heraclitus R.E.Hobart Thomas Hobbes David Hodgson Shadsworth Hodgson Baron d'Holbach Ted Honderich Pamela Huby David Hume Ferenc Huoranszki Frank Jackson William James Lord Kames Robert Kane Immanuel Kant Tomis Kapitan Walter Kaufmann Jaegwon Kim William King Hilary Kornblith Christine Korsgaard Saul Kripke Thomas Kuhn Andrea Lavazza Christoph Lehner Keith Lehrer Gottfried Leibniz Jules Lequyer Leucippus Michael Levin Joseph Levine George Henry Lewes C.I.Lewis David Lewis Peter Lipton C. Lloyd Morgan John Locke Michael Lockwood Arthur O. Lovejoy E. Jonathan Lowe John R. Lucas Lucretius Alasdair MacIntyre Ruth Barcan Marcus Tim Maudlin James Martineau Nicholas Maxwell Storrs McCall Hugh McCann Colin McGinn Michael McKenna Brian McLaughlin John McTaggart Paul E. Meehl Uwe Meixner Alfred Mele Trenton Merricks John Stuart Mill Dickinson Miller G.E.Moore Thomas Nagel Otto Neurath Friedrich Nietzsche John Norton P.H.NowellSmith Robert Nozick William of Ockham Timothy O'Connor Parmenides David F. Pears Charles Sanders Peirce Derk Pereboom Steven Pinker Plato Karl Popper Porphyry Huw Price H.A.Prichard Protagoras Hilary Putnam Willard van Orman Quine Frank Ramsey Ayn Rand Michael Rea Thomas Reid Charles Renouvier Nicholas Rescher C.W.Rietdijk Richard Rorty Josiah Royce Bertrand Russell Paul Russell Gilbert Ryle JeanPaul Sartre Kenneth Sayre T.M.Scanlon Moritz Schlick Arthur Schopenhauer John Searle Wilfrid Sellars Alan Sidelle Ted Sider Henry Sidgwick Walter SinnottArmstrong J.J.C.Smart Saul Smilansky Michael Smith Baruch Spinoza L. Susan Stebbing Isabelle Stengers George F. Stout Galen Strawson Peter Strawson Eleonore Stump Francisco Suárez Richard Taylor Kevin Timpe Mark Twain Peter Unger Peter van Inwagen Manuel Vargas John Venn Kadri Vihvelin Voltaire G.H. von Wright David Foster Wallace R. Jay Wallace W.G.Ward Ted Warfield Roy Weatherford C.F. von Weizsäcker William Whewell Alfred North Whitehead David Widerker David Wiggins Bernard Williams Timothy Williamson Ludwig Wittgenstein Susan Wolf Scientists David Albert Michael Arbib Walter Baade Bernard Baars Jeffrey Bada Leslie Ballentine Marcello Barbieri Gregory Bateson John S. Bell Mara Beller Charles Bennett Ludwig von Bertalanffy Susan Blackmore Margaret Boden David Bohm Niels Bohr Ludwig Boltzmann Emile Borel Max Born Satyendra Nath Bose Walther Bothe Jean Bricmont Hans Briegel Leon Brillouin Stephen Brush Henry Thomas Buckle S. H. Burbury Melvin Calvin Donald Campbell Sadi Carnot Anthony Cashmore Eric Chaisson Gregory Chaitin JeanPierre Changeux Rudolf Clausius Arthur Holly Compton John Conway Jerry Coyne John Cramer Francis Crick E. P. Culverwell Antonio Damasio Olivier Darrigol Charles Darwin Richard Dawkins Terrence Deacon Lüder Deecke Richard Dedekind Louis de Broglie Stanislas Dehaene Max Delbrück Abraham de Moivre Bernard d'Espagnat Paul Dirac Hans Driesch John Eccles Arthur Stanley Eddington Gerald Edelman Paul Ehrenfest Manfred Eigen Albert Einstein George F. R. Ellis Hugh Everett, III Franz Exner Richard Feynman R. A. Fisher David Foster Joseph Fourier Philipp Frank Steven Frautschi Edward Fredkin Benjamin GalOr Howard Gardner Lila Gatlin Michael Gazzaniga Nicholas GeorgescuRoegen GianCarlo Ghirardi J. Willard Gibbs James J. Gibson Nicolas Gisin Paul Glimcher Thomas Gold A. O. Gomes Brian Goodwin Joshua Greene Dirk ter Haar Jacques Hadamard Mark Hadley Patrick Haggard J. B. S. Haldane Stuart Hameroff Augustin Hamon Sam Harris Ralph Hartley Hyman Hartman Jeff Hawkins JohnDylan Haynes Donald Hebb Martin Heisenberg Werner Heisenberg John Herschel Basil Hiley Art Hobson Jesper Hoffmeyer Don Howard John H. Jackson William Stanley Jevons Roman Jakobson E. T. Jaynes Pascual Jordan Eric Kandel Ruth E. Kastner Stuart Kauffman Martin J. Klein William R. Klemm Christof Koch Simon Kochen Hans Kornhuber Stephen Kosslyn Daniel Koshland Ladislav Kovàč Leopold Kronecker Rolf Landauer Alfred Landé PierreSimon Laplace Karl Lashley David Layzer Joseph LeDoux Gilbert Lewis Benjamin Libet David Lindley Seth Lloyd Hendrik Lorentz Josef Loschmidt Ernst Mach Donald MacKay Henry Margenau Owen Maroney Humberto Maturana James Clerk Maxwell Ernst Mayr John McCarthy Warren McCulloch N. David Mermin George Miller Stanley Miller Ulrich Mohrhoff Jacques Monod Vernon Mountcastle Emmy Noether Alexander Oparin Abraham Pais Howard Pattee Wolfgang Pauli Massimo Pauri Roger Penrose Steven Pinker Colin Pittendrigh Max Planck Susan Pockett Henri Poincaré Daniel Pollen Ilya Prigogine Hans Primas Henry Quastler Adolphe Quételet Pasco Rakic Lord Rayleigh Jürgen Renn Emil Roduner Juan Roederer Jerome Rothstein David Ruelle Tilman Sauer Jürgen Schmidhuber Erwin Schrödinger Aaron Schurger Sebastian Seung Thomas Sebeok Franco Selleri Claude Shannon Charles Sherrington David Shiang Abner Shimony Herbert Simon Dean Keith Simonton Edmund Sinnott B. F. Skinner Lee Smolin Ray Solomonoff Roger Sperry John Stachel Henry Stapp Tom Stonier Antoine Suarez Leo Szilard Max Tegmark Teilhard de Chardin Libb Thims William Thomson (Kelvin) Richard Tolman Giulio Tononi Peter Tse Francisco Varela Vlatko Vedral Mikhail Volkenstein Heinz von Foerster Richard von Mises John von Neumann Jakob von Uexküll C. S. Unnikrishnan C. H. Waddington John B. Watson Daniel Wegner Steven Weinberg Paul A. Weiss Herman Weyl John Wheeler Wilhelm Wien Norbert Wiener Eugene Wigner E. O. Wilson Günther Witzany Stephen Wolfram H. Dieter Zeh Ernst Zermelo Wojciech Zurek Konrad Zuse Fritz Zwicky Presentations Biosemiotics Free Will Mental Causation James Symposium 
Albert Einstein
We will show that in the two decades preceding the "founding" of quantum mechanics by Niels Bohr, Werner Heisenberg, Max Born, Pascual Jordan, P. A. M. Dirac, Erwin Schrödinger, and Wolfgang Pauli, Einstein discovered ontological chance in quantum physics, without which no new information can be created. Without chance and new information, there can be no "free creations of the human mind," which Einstein correctly recognized as the fundamental source of new scientific theories.
Einstein saw a wave randomly "collapse" twenty years before there was a "wave function" and the Schrödinger wave equation. He discovered the existence of indeterministic chance as a "weakness" in quantum theory over a decade before Heisenberg published his uncertainty principle.
Since the validity of any theory rests on its experimental confirmation, as Einstein knew very well, we can say that the extraordinary confirmation of quantum mechanics, especially its probabilistic nature, makes it the best supported theory in the history of science, but nevertheless it is a statistical theory.
He deplored his discoveries. Paradoxically, ironically perhaps, and even tragically, only a handful of scientists and philosophers recognize the full range of Einstein's contributions, primarily because he disavowed his own quantum discoveries as contrary to his fundamental beliefs about the workings of the universe. Few of us are immune to the power of beliefs that prevent the acceptance of scientifically established facts. As exceptional a scientist as Einstein was, he was no exception there. Randomness was not his only concern, maybe not even his main concern, as we shall see. Quantum mechanics appears to conflict with special relativity, and its nonlocality may conflict with general relativity and Einstein's dream of a "unified field theory." All his life, Einstein had grave doubts about field theories. They became more extreme in his later years, when he wrote
One can give good reasons why reality cannot at all be represented by a continuous field. From the quantum phenomena it appears to follow with certainty that a finite system of finite energy can be completely described by a finite set of numbers (quantum numbers). This does not seem to be in accordance with a continuum theory, and must lead to an attempt to find a purely algebraic theory for the description of reality. But nobody knows how to obtain the basis of such a theory. In principle, continuous field theories contain an infinite amount of information. The differential equations that describe classical physics in space and time assume there are an infinite number of infinitesimal points along any finite line segment. But Einstein saw that any finite volume (even the whole observable universe) can contain only a finite number of discrete quanta of matter or energy. Quantum mechanics can thus in principle be described with simpler difference equations in what Einstein described as an "algebraic" theory. Ludwig Boltzmann had shown that he could derive his entropy law assuming that space can be described as "coarse grained" into small enough discrete volumes, though still large enough to contain many particles. Quite apart from his great deterministic and continuous theories of special and general relativity, Einstein was one of the most important creators (both discoverer and inventor) of the indeterministic and discrete theory of quantum mechanics. In his 1905 paper on the lightquantum hypothesis and photoelectric effect, he quantized the radiation field, where Max Planck had only quantized the energy in his virtual oscillators. Einstein was first to see that electromagnetic radiation is particulate. And in his very next paper he proved the existence of atoms. In that one year he saw both matter and energy as particulate and how they are converted into one another, E = mc^{2}. Einstein thus saw that both the material and the energetic universe have discrete and discontinuous properties! His 1905 paper on Brownian motion predicted sizes and motions for atoms that were confirmed just a few years later. And although he waited ten years to do so, Einstein stated unequivocally that quantum processes are fundamentally indeterministic, a matter of chance. "A weakness in the theory," he called it in 1916. He lamented at that time to his friend Michele Besso that he was the only scientist who believed in the reality of what we now call photons, "I do not doubt anymore the reality of radiation quanta, although I still stand quite alone in this conviction." On a careful reading of his 1905 photoelectric effect paper, we can see that Einstein was already concerned about fasterthanlight actions, thirty years before his EinsteinPodolskyRosen paper popularized the mysteries and paradoxes of quantum nonlocality and entanglement. We hope to show that many of today's controversies in the interpretations of quantum mechanics can be resolved by seeing these problems through Einstein's eyes. Despite his foundational work quantizing radiation, Einstein rarely gets any credit for his contributions to quantum mechanics. There are a number of important reasons for this, which lead historians of quantum theory to start with Planck's quantum of action, then jump over Einstein's 1905 papers and his 1909 work on waveparticle duality to Niels Bohr's "old quantum theory" of the atom in 1913. Today, Bohr's "quantum jump" of an electron between stationary states is described as emitting or absorbing a "photon" of energy hν. In actuality, Bohr fought against Einstein's lightquantum hypothesis and denied the existence of photons until the mid1920's. Bohr's work in 1924 with H. A. Kramers and John Slater was the last defense of continuous, as opposed to discrete, radiation. The BohrKramersSlater theory claimed that energy was not conserved in each matterradiation interaction, but only conserved statistically. Immediately, Einstein suggested multiple experiments to Walther Bothe that could disprove the BKS claim. In 1925, Bothe and Hans Geiger developed two experiments that disproved the BKS theory. At this point, Bohr finally accepted, though never enthusiastically, Einstein's light quanta as real, twenty years after Einstein's insight in his 1905 "miracle year." Besides quantizing light energy and seeing its interchangeability with matter, E = mc^{2}, Einstein was the first scientist to see many of the most fundamental aspects of quantum physics, e.g., nonlocality and instantaneous actionatadistance (1905), waveparticle duality (1909), emission and absorption processes that introduce indeterminism and acausality whenever matter and radiation interact (191617.) He predicted the stimulated emission of radiation behind today's lasers, the indistinguishability of elementary particles with their strange quantum statistics (1925), and the nonseparability and entanglement of interacting identical particles (1935). Just because Einstein did not regard any of these discoveries as part of a fundamental "local" reality that Einstein wanted is no reason to deny him credit for them all. Einstein's description of waveparticle duality is as good as anything written today. He saw the relation between the wave and the particle as the relation between probable possibilities and the realization of one possibility as an actual event. He saw the wave spreading out in space and giving us the probability of finding a particle in different locations. Where Einstein saw the particle as concrete and material, he described the wave as a "ghostly field," which is exactly right according to the information interpretation of quantum mechanics. The wave is neither matter nor energy, but pure abstract information about locating concrete matter and energy. The information about probabilities and possibilities in the wave function is immaterial, but that abstract information has real causal powers. The wave's interference with itself predicts null points where no particles should be found. And experiments confirm that no particles are found there. Immaterial information is a kind of modern "spirit." Einstein also described the wave function as a ""guiding field" (Führungsfeld), an idea taken up later by Louis de Broglie as his "pilot waves." Following de Broglie, Schrödinger developed his equation that gives us the value of the wave function ψ at each point and describes how the probabilityamplitude wave function moves through space deterministically. This restoration of some determinism was a brief bright moment for Einstein. He saw a possible return to a deterministic theory for quantum mechanics and his continuous field theory. But it was not to be, despite the large number of presentday physicists who are still pursuing Einstein's and Schrödinger's deterministic dreams, by denying indeterminism and "quantum jumping." The linearity of the Schrödinger wave equation produces the mysterious superposition of states and the projection postulate  the wave function "collapse." In a linear equation, the sum of two solutions is also a solution. Although the projection postulate is basically a formalization of Einstein's 1916 transition probabilities from an excited state to more than one lower state, although he had been first to see a light wave collapse into a photon that could eject an electron in his 1905 photoelectric effect paper, and although he had been first to proclaim ontological chance as a part of the quantum theory, it must have been a disappointment to Einstein to find that the determinism in Schrödinger's wave equation could only determine his probabilities and that ontological chance is still real. Einstein could never accept most of his quantum discoveries because they conflicted with his basic idea that nature is best described by a continuous field theory using partial differential equations that are functions of "local" variables, primarily the spacetime fourvector of his general relativistic theory. Einstein's idea of a "local" reality is one where "actionatadistance" is limited to causal effects that propagate at or below the speed of light, according to his theory of relativity. Einstein believed that quantum theory, as good as it is (and he never saw anything better), is "incomplete." This is so, because its statistical predictions (phenomenally accurate in the limit of large numbers of identical experiments  "ensembles" Einstein called them), tell us nothing but "probabilities" about individual systems. Even worse, he saw that the wave functions of entangled twoparticle systems predict fasterthanlight correlations of properties between events in a spacelike separation. He mistakenly thought this violated his theory of relativity. Although this was the heart of his famous EPR paradox paper in 1935, we shall see that Einstein was already concerned about fasterthanlight transfer of energy and that he saw spherical light waves "collapsing" instantaneously in his very first paper on quantum theory. In most general histories, and in the brief histories included in modern quantum mechanics textbooks, the problems raised by Einstein are usually presented as arising after the "founders" of quantum mechanics and their Copenhagen Interpretation in the late 1920's. Modern attention to Einstein's work on quantum physics often starts with the EinsteinPodolskyRosen paper of 1935, when the mysteries of nonlocality, nonseparability, and entanglement are first clearly understood by Einstein's opponents. Physicists today think of quantum mechanics as beginning with the Heisenberg (particle) formulation and the Schrödinger (wave) formulation. The popular image of Einstein postEPR is either in the role of critic trying to expose fundamental flaws in the "new" quantum mechanics or as an old man who simply didn't understand the new quantum theory. Both these images of Einstein are seriously flawed, as we shall see. Many histories of quantum theory, most starting from the Copenhagen perspective of Bohr, Heisenberg, Born, Jordan, and Pauli, focus on Einstein's failed attempts in debates with Bohr to challenge the uncertainty principle. EPR is described as failing to show that quantum mechanics is "incomplete." This is a verbal quibble. Quantum mechanics is indeed incomplete in that it cannot predict simultaneously the position and momentum of a particle, nor the "real" path of a particle between measurements. Most important, QM is only a statistical theory, as Einstein maintained. Its results are only confirmed by large numbers of identical experiments. Continuous matter and radiation only appear when we average over large numbers of discrete particles. Few histories point out that it was Einstein who over three decades invented (or discovered) nonlocality and entanglement, as well as the ontological chance in quantum mechanics that is the real basis of the acausality that Heisenberg later saw in his uncertainty principle.
The LightQuantum Hypothesis (1905)
The Photoelectric Effect (1905)
Einstein had very strong reasons for imagining that light must be concentrated in a physically localized bundle of energy. He described it in section 8 of this same paper, explaining the photoelectric effect, the emission of electrons from surfaces illuminated by radiation. He wrote: The usual conception, that the energy of light is continuously distributed over the space through which it propagates, encounters very serious difficulties when one attempts to explain the photoelectric phenomena, as has been pointed out in Herr Lenard's pioneering paper.Einstein shows here that the whole energy of an incident light quantum is absorbed by a single electron. Some of that energy is P, the work needed to escape from the metal. The rest is the kinetic energy E = ½ m v^{2} of the electron. Einstein's "photoelectric equation" is
E = hν  P
This equation predicts a linear relationship between the frequency of Einstein's light quantum hν, and the energy E of the ejected electron. It wasn't until ten years later that R. A. Millikan confirmed Einstein's photoelectric equation. Millikan nevertheless denied that it proved Einstein's radical but clairvoyant ideas about light quanta! If the energy travels as a spherical light wave radiated into space in all directions, how can it instantaneously collect itself together to be absorbed into a single electron. Einstein already in 1905 sees something nonlocal about the photon and that there is both a wave aspect and a particle aspect to electromagnetic radiation. He will make those aspects more clear and in 1909 describe the waveparticle relationship more clearly than it is usually presented today, with all the confusion about whether photons and electrons are waves or particles or both.
Waveparticle duality (1909)
Einstein greatly expanded his lightquantum hypothesis in a presentation at the Salzburg conference in September, 1909. He argued that the interaction of radiation and matter involves elementary processes that are not "invertible," a deep insight into the irreversibility of natural processes. While incoming spherical waves of radiation are mathematically possible, they are not practically achievable. Nature appears to be asymmetric in time. He speculates that the continuous electromagnetic field might be made up of large numbers of light quanta  singular points in a field that superimpose collectively to create the wavelike behavior. Although he could not formulate a mathematical theory that does justice to both the continuous oscillatory waves and the discrete particle pictures, Einstein argued that they could be "fused" and made compatible. This was over a decade before Erwin Schrödinger's wave mechanics and Werner Heisenberg's quantum mechanics. And because gases behave statistically, he knows that the connection between the wave and particles may involve probabilistic behavior.
When light was shown to exhibit interference and diffraction, it seemed almost certain that light should be considered a wave.
The Emission and Absorption of Radiation (1916)
When he finished the years needed to complete his general theory of relativity, Einstein turned back to quantum theory and to Bohr's 1913 postulates about electrons jumping between stationary (nonradiating) states and radiating energy E_{m}  E_{n} = hν. Where Bohr's two postulates provided amazingly accurate explanations of the Balmer and Lyman lines in the hydrogen spectrum, Einstein showed how to derive those postulates along with his latest, and so far simplest, derivation of the Planck radiation law.
Where Bohr and Planck had manipulated mathematical expressions to correspond with spectroscopic data, Einstein found the statistical probabilities for absorption and emission of light quanta when an electron jumps between discrete energy states, showing his deep physical understanding of interactions between electrons and radiation, going back over ten years. He predicted the existence of "stimulated emission" and showed quantum theory is the source of ontological chance.
At this time, Einstein felt very much alone in believing the reality (his emphasis) of light quanta: I do not doubt anymore the reality of radiation quanta, although I still stand quite alone in this conviction Einstein derived "transition probabilities" for quantum jumps, described as A and B coefficients for the processes of absorption, spontaneous emission, and (his newly predicted) stimulated emission of radiation. In two papers, "Emission and Absorption of Radiation in Quantum Theory," and "On the Quantum Theory of Radiation," he again derived the Planck law (for Planck it was mostly a guess at the formula needed to fit spectroscopic observations), he derived Planck's postulate E = hν, and he derived Bohr's second postulate E_{m}  E_{n} = hν. Einstein did this by exploiting the obvious relationship between the MaxwellBoltzmann distribution of gas particle velocities and the distribution of radiation in Planck's law. The formal similarity between the chromatic distribution curve for thermal radiation and the Maxwell velocitydistribution law is too striking to have remained hidden for long. In fact, it was this similarity which led W. Wien, some time ago, to an extension of the radiation formula in his important theoretical paper, in which he derived his displacement law...Not long ago I discovered a derivation of Planck's formula which was closely related to Wien's original argument and which was based on the fundamental assumption of quantum theory. This derivation displays the relationship between Maxwell's curve and the chromatic distribution curve and deserves attention not only because of its simplicity, but especially because it seems to throw some light on the mechanism of emission and absorption of radiation by matter, a process which is still obscure to us.But the introduction of MaxwellBoltzmann statistical mechanical thinking to electromagnetic theory has produced what Einstein called a "weakness in the theory." It introduces the reality of an irreducible objective chance! If light quanta are particles with energy E = hν traveling at the velocity of light c, then they should have a momentum p = E/c = hν/c. When light is absorbed by material particles, this momentum will clearly be transferred to the particle. But when light is emitted by an atom or molecule, a problem appears.
The "statistical interpretation" of Max Born tells us the outgoing wave is the probability amplitude wave function Ψ, whose absolute square is the probability of finding a light particle in an arbitrary direction, as Einstein qualitatively knew well but never published.
Conservation of momentum requires that the momentum of the emitted particle will cause an atom to recoil with momentum hν/c in the opposite direction. However, the standard theory of spontaneous emission of radiation is that it produces a spherical wave going out in all directions. A spherically symmetric wave has no preferred direction. In which direction does the atom recoil? Einstein asked:
Does the molecule receive an impulse when it absorbs or emits the energy ε? For example, let us look at emission from the point of view of classical electrodynamics. When a body emits the radiation ε it suffers a recoil (momentum) ε/c if the entire amount of radiation energy is emitted in the same direction. If, however, the emission is a spatially symmetric process, e.g., a spherical wave, no recoil at all occurs. This alternative also plays a role in the quantum theory of radiation. When a molecule absorbs or emits the energy ε in the form of radiation during the transition between quantum theoretically possible states, then this elementary process can be viewed either as a completely or partially directed one in space, or also as a symmetrical (nondirected) one. It turns out that we arrive at a theory that is free of contradictions, only if we interpret those elementary processes as completely directed processes.But the inability to predict both the time and direction of light particle emissions, said Einstein in 1917, is "a weakness in the theory..., that it leaves time and direction of elementary processes to chance (Zufall, ibid.)." It is only a weakness for Einstein, of course, because his God does not play dice.One can give good reasons why reality cannot at all be represented by a continuous field. From the quantum phenomena it appears to follow with certainty that a finite system of finite energy can be completely described by a finite set of numbers (quantum numbers). This does not seem to be in accordance with a continuum theory, and must lead to an attempt to find a purely algebraic theory for the description of reality. But nobody knows how to obtain the basis of such a theory.It speaks in favor of the theory that the statistical law assumed for [spontaneous] emission is nothing but the Rutherford law of radioactive decay. Einstein clearly saw, as none of his contemporaries did, that since spontaneous emission is a statistical process, it cannot possibly be described with classical physics. The properties of elementary processes required...make it seem almost inevitable to formulate a truly quantized theory of radiation. Einstein may not have liked this conceptual crisis, but his insights into the indeterminism involved in quantizing matter and energy were known, if largely ignored, for another decade until Heisenberg's quantum theory introduced his famous uncertainty principle in 1927. Heisenberg states that the exact position and momentum of an atomic particle can only be known within certain (sic) limits. The product of the position error and the momentum error is greater than or equal to Planck's constant h/2π.
ΔpΔx ≥ h/2π
The Interaction of Radiation and Matter as the Origin of Irreversibility (1916)
In his two papers on quantum mechanics in 191617, Einstein's discovery of ontological chance is the most important contribution to physics and philosophy. But his insight into the asymmetry of the emission and absorption processes may be used to discover the origin of irreversibility and an explanation for Boltzmann's hypothesis of "molecular disorder." What we might call Einstein's "radiation asymmetry" was introduced with these words, When a molecule absorbs or emits the energy ε in the form of radiation during the transition between quantum theoretically possible states, then this elementary process can be viewed either as a completely or partially directed one in space, or also as a symmetrical (nondirected) one. It turns out that we arrive at a theory that is free of contradictions, only if we interpret those elementary processes as completely directed processes. The elementary process of the emission and absorption of radiation is asymmetric, because the process is directed, as Einstein had explicitly noted first in 1909, and we know he had seen as early as 1905. The apparent isotropy of the emission of radiation is only what Einstein called "pseudoisotropy" (Pseudoisotropie), a consequence of time averages over large numbers of events. Einstein often substitutes time averages for space averages, or averages over the possible states of a system in statistical mechanics.
a quantum theory free from contradictions can only be obtained if the emission process, just as absorption, is assumed to be directional. In that case, for each elementary emission process Z_{m}>Z_{n} a momentum of magnitude (ε_{m}—ε_{n})/c is transferred to the molecule. If the latter is isotropic, we shall have to assume that all directions of emission are equally probable. Now the principle of microscopic reversibility is a fundamental assumption of statistical mechanics. It underlies the principle of "detailed balancing," which is critical to the understanding of chemical reactions. In thermodynamic equilibrium, the number of forward reactions is exactly balanced by the number of reverse reactions. But microscopic reversibility, while true in the sense of averages over time, should not be confused with the reversibility of individual collisions between molecules. The equations of classical dynamics are reversible in time. And the deterministic Schrödinger equation of motion in quantum mechanics is also time reversible. Irreversibility thus depends on the "projection" of a superposition of states into a single state, the socalled "collapse" of the wave function.
The Quantum Statistics for Photons (1924)
In 1924, Einstein received an amazing very short paper from India by Satyendra Nath Bose. Einstein must have been pleased to read the title, "Planck's Law and the Hypothesis of Light Quanta." It was more attention to Einstein's 1905 work than anyone had paid in nearly twenty years. The paper began by claiming that the "phase space" (a combination of 3dimensional coordinate space and 3dimensional momentum space) should be divided into small volumes of h^{3}, the cube of Planck's constant. By counting the number of possible distributions of light quanta over these cells, Bose claimed he could calculate the entropy and all other thermodynamic properties of the radiation.
Bose easily derived the inverse exponential function, Einstein too had derived this. Maxwell and Boltzmann derived it, without the additional 1, by analogy from the Gaussian exponential tail of probability and the theory of errors.
1 / (e^{  hν / kT } 1)
(Planck had simply guessed this expression from Wien's law by adding the term  1 in the denominator of Wien's a / e^{  bν / T}). All previous derivations of the Planck law, including Einstein's of 191617 (which Bose called "remarkably elegant"), used classical electromagnetic theory to derive the density of radiation, the number of "modes" or "degrees of freedom" of the radiation field,
ρ_{ν}dν = (8πν^{2}dν / c^{3}) E
But now Bose showed he could get this quantity with a simple statistical mechanical argument remarkably like that Maxwell used to derive his distribution of molecular velocities. Where Maxwell said that the three directions of velocities for particles are independent of one another, but of course equal to the total momentum,
p_{x2} + p_{y2} + p_{z2} = p^{2} ,
Bose just used Einstein's relation for the momentum of a photon,
p = hν / c,
and he wrote
p_{x2} + p_{y2} + p_{z2} = h^{2}ν^{2} / c^{2} .
This led him to calculate a frequency interval in phase space as
∫ dx dy dz dp_{x} dp_{y} dp_{z} = 4πV ( hν / c )^{3} ( h dν / c ) = 4π ( h^{3} ν^{2} / c^{3} ) V dν,
which he simply divided by h^{3}, multiplied by 2 to account for two polarization degrees of freedom, and he had derived the number of cells belonging to dν,
ρ_{ν}dν = (8πν^{2}dν / c^{3}) E ,
without using classical radiation laws, a correspondence principle, or even Wien's law. His derivation was purely statistical mechanical, based only on the number of cells in phase space and the number of ways N photons can be distributed among them. Einstein immediately translated the Bose paper into German and had it published in Zeitschrift für Physik, without even telling Bose. More importantly, Einstein then went on to discuss a new quantum statistics that predicted lowtemperature condensation of any particles with integer values of the spin. So called BoseEinstein statistics were quickly shown by Dirac to lead to the quantum statistics of halfinteger spin particles called FermiDirac statistics. Fermions are halfinteger spin particles that obey Pauli's exclusion principle so a maximum of two particles, with opposite spins, can be found in the fundamental h^{3} volume of phase space identified by Bose. Einstein's 1916 work on transition probabilities predicted the stimulated emission of radiation that brought us lasers (light amplification by the stimulated emission of radiation). Now his work on quantum statistics brought us the BoseEinstein condensation. Either work would have made their discoverer a giant in physics, but these are more often attributed to Bose, just as Einstein's quantum discoveries before the Copenhagen Interpretation are mostly forgotten by historians and today's textbooks, or attributed to others. This may have been Einstein's last positive contribution to quantum physics. Some judge his next efforts as purely negative attempts to discredit quantum mechanics, by graphically illustrating quantum phenomena that seem logically impossible or at least in violation of fundamental theories like his relativity. But information philosophy hopes to provide explanations for Einstein's paradoxes that depend on the immaterial nature of information. The phenomena of nonlocality, nonseparability, and entanglement may not be made intuitive by our explanations, but they can be made understandable. And they can be visualized in a way that Einstein and Schrödinger might have liked, even if they might still have found the phenomena difficult to believe. We hope even the layperson will see our animations as providing them an understanding of what quantum mechanics is doing in the microscopic world. The animations present standard quantum physics as Einstein saw it, though Schrödinger never accepted the "collapse" of the wave function and the existence of particles making quantum jumps.
The Fifth Solvay Conference, On Electrons and Photons (1927)
Sadly, despite Einstein's two decades of pioneering work on the interaction of photons and electrons, his ideas and concerns were given little attention at this Solvay, though the conference was dedicated to electrons and photons.
The conference was dominated by papers on the new quantum theory delivered by Louis de Broglie, Niels Bohr, Max Born and Werner Heisenberg. It is best known for Einstein's afterhours suggestions to Niels Bohr and Werner Heisenberg probing for faults in the uncertainty principle. Accounts of these events have been told largely by the victors (there are no holes in uncertainty) but Einstein has said they often missed or ignored his important point. That point was the nonlocal behavior of a spherical light wave as it collapses to get absorbed by a single electron. This was Einstein's only contribution mentioned in the published proceedings. Here are the notes on Einstein's original remarks at the conference and Bohr's brief response. They contain much of Einstein's 1935 EPR paper, except in 1927 only one particle is involved. Entanglement in EPR requires two identical particles. Notice how Einstein's diagram clearly shows his concerns of over two decades about reconciling a spherical wave (his example is now an electron) and its collapse to being measured at just one point as if it is a particle. At this point in the history of quantum mechanics, waveparticle duality is seen as the debate between Schrödinger's wave mechanics and Heisenberg's particle mechanics.
Bohr's reaction to Einstein's presentation has been preserved. He didn't understand a word! He disingenuously claims he does not know what quantum mechanics is. His response is vague and ends with his ideas on complementarity and the inability to describe a causal spacetime reality.
Twentytwo years later, in his contribution to the Schilpp memorial volume on Einstein, Bohr had no better response to Einstein's 1927 concerns. But he does remember vividly and provides a picture of what Einstein drew on the blackboard. Here is Bohr's 1949 recollection:
At the general discussion in Como, we all missed the presence of Einstein, but soon after, in October 1927, I had the opportunity to meet him in Brussels at the Fifth Physical Conference of the Solvay Institute, which was devoted to the theme "Electrons and Photons." Although Bohr seems to have missed Einstein's point completely, Werner Heisenberg at least came to explain it well. In his 1930 lectures at the University of Chicago, Heisenberg presented a critique of both particle and wave pictures, including a new example of nonlocality that Einstein had apparently developed since 1927. It includes Einstein's concern about "actionatadistance" that might violate his principle of relativity, and anticipates the EinsteinPodolskyRosen paradox. Heisenberg wrote: In relation to these considerations, one other idealized experiment (due to Einstein) may be considered. We imagine a photon which is represented by a wave packet built up out of Maxwell waves. It will thus have a certain spatial extension and also a certain range of frequency. By reflection at a semitransparent mirror, it is possible to decompose it into two parts, a reflected and a transmitted packet. There is then a definite probability for finding the photon either in one part or in the other part of the divided wave packet. After a sufficient time the two parts will be separated by any distance desired; now if an experiment yields the result that the photon is, say, in the reflected part of the packet, then the probability of finding the photon in the other part of the packet immediately becomes zero. The experiment at the position of the reflected packet thus exerts a kind of action (reduction of the wave packet) at the distant point occupied by the transmitted packet, and one sees that this action is propagated with a velocity greater than that of light. However, it is also obvious that this kind of action can never be utilized for the transmission of signals so that it is not in conflict with the postulates of the theory of relativity.
Einstein visualizes TwoParticle Nonlocality (1933)
In 1933, shortly before he left Germany to emigrate to America,
Einstein attended a lecture on quantum electrodynamics by Leon
Rosenfeld. Keep in mind that Rosenfeld was perhaps the most
dogged defender of the Copenhagen Interpretation. After the talk,
Einstein asked Rosenfeld,
“What do you think of this situation?” Suppose two particles are set in motion towards each other with the same, very large, momentum, and they interact with each other for a very short time when they pass at known positions. Consider now an observer who gets hold of one of the particles, far away from the region of interaction, and measures its momentum: then, from the conditions of the experiment, he will obviously be able to deduce the momentum of the other particle. If, however, he chooses to measure the position of the first particle, he will be able tell where the other particle is. It is most unfortunate that Einstein did not explain that measuring the momentum of the first particle allows us to deduce the momentum of the second particle because of the conservation of linear momentum. The same conservation principle explains as Einstein says, "If, however, he chooses to measure the position of the first particle, he will be able tell where the other particle is." If Einstein had called this ability to tell "knowledge (information) at a distance," instead of "spooky action at a distance," entanglement might never have been thought "spooky" at all, just a correlation of properties. We can diagram a simple case of Einstein’s question as follows after the particles have interacted and separate from the center. We use electrons instead of generic particles, an anachronism introduced by David Bohm in 1952.
Recall that it was Einstein who discovered in 1924 the identical nature, indistinguishability, and interchangeability of some quantum particles. He found that identical particles are not independent, altering their quantum statistics.
After the particles interact at t_{1}, quantum mechanics describes them with a single twoparticle wave function that is not the product of independent singleparticle wave functions. In the case of electrons, which are indistinguishable interchangeable particles, it is not proper to say electron 1 goes this way and electron 2 that way. (Nevertheless, it is convenient to label the particles, as we do in the illustration.)
Note the anachronism of electrons as Einstein's generic particles. It was David Bohm in 1952 who proposed that Einstein's EPR problem use electrons. Today many if not most accounts of the EPR paradox describe it with electrons. Einstein then asked Rosenfeld, “How can the final state of the second particle be influenced by a measurement performed on the first after all interaction has ceased between them?” This was the germ of the EPR paradox, and ultimately the problem of twoparticle entanglement. Why does Einstein question Rosenfeld and describe this as an “influence,” suggesting an “actionatadistance?” It is only paradoxical in the context of Rosenfeld’s Copenhagen Interpretation, since the second particle is not itself measured and yet we know something about its properties, which the Copenhagen Interpretation says we cannot know without an explicit measurement.. Einstein was clearly correct to tell Rosenfeld that at a later time t_{2}, a measurement of one particle's position would instantly establish the position of the other particle  without measuring it. Einstein simply used conservation of linear momentum implicitly to calculate (and know) the position of the second particle. Two years later, reacting to EPR, Schrödinger described two such particles as becoming "entangled" (verschränkt) at their first interaction, so "nonlocal" phenomena are also known as "quantum entanglement." Although conservation laws are rarely cited as the explanation, they are the physical reason that entangled particles always produce correlated results for all properties. If the results were not always correlated, the implied violation of a fundamental conservation law would cause a much bigger controversy than entanglement itself, as puzzling as that is.
Einstein Accepts Quantum Mechanics But Still Hopes For A Continuum Theory (1934)
In 1934, Einstein described one way to reconcile nonlocality with a fourdimensional spacetime continuum theory. At this time, Einstein is clearly supportive of Heisenberg's uncertainty principle and the probabilistic nature of quantum theory:
EinsteinPodolskyRosen and Entanglement (1935)
Einstein and colleagues Boris Podolsky and Nathan Rosen, proposed in 1935 a paradox (known by their initials as EPR or as the EinsteinPodolsyRosen paradox) to exhibit internal contradictions in the new quantum physics. They hoped to show that quantum theory could not describe certain intuitive "elements of reality" and thus was incomplete. They said that, as far as it goes, quantum mechanics is correct, just not "complete."
Einstein was correct that quantum theory is "incomplete" relative to classical physics, which has twice as many dynamical variables that can be known with arbitrary precision. But half of this information is missing in quantum physics, due to the indeterminacy principle which allows only one of each pair of noncommuting observables (for example momentum or position) to be known with arbitrary accuracy. Even more important, an individual particle, cannot be said to have a known position before a measurement, since evolution described by the unitary and deterministic Schrödinger equation provides us only probabilities. The most that can be said is that the particle can be found anywhere the probability amplitude is nonzero. This was the core idea of Einstein's claim of "incompleteness." For Bohr to deny this and call quantum mechanics "complete" was just to play word games, which infuriated Einstein. Einstein was also correct that indeterminacy makes quantum theory an irreducibly discontinuous and statistical theory. Its predictions and highly accurate experimental results are statistical in that they depend on an ensemble of identical experiments, not on any individual experiment. Einstein wanted physics to be a continuous field theory, in which all physical variables are completely and locally determined by the fourdimensional field of spacetime in his theory of relativity. Einstein and his colleagues Erwin Schrödinger, Max Planck, (later David Bohm), and others hoped for a return to deterministic physics, and the elimination of mysterious quantum phenomena like the superposition of states, the mysterious "collapse" of the wave function, and Schrödinger's famous cat. EPR continues to fascinate determinist philosophers of science who hope to prove that quantum indeterminacy does not exist.
What happens according to the information interpretation of quantum mechanics is an instantaneous change in the information about probabilities (actually complex probability amplitudes). Nothing physical (matter or energy) is moving anywhere.
But Einstein was also bothered by what is known as "nonlocality," as we saw at the 1927 Solvay conference. This mysterious phenomenon was even more clearly exhibited in EPR experiments as the apparent transfer of something physical faster than the speed of light. Einstein may have already seen this inconsistency with his relativity theory in his 1905 papers.
The 1935 EPR paper was based on a question of Einstein's about two electrons fired in opposite directions from a central source with equal velocities. He imagined them starting at t_{0} some distance apart and approaching one another with high velocities. Then for a short time interval from t_{1} to t_{1} + Δt the particles are in contact with one another.
Most accounts of entanglement and nonlocality begin with the idea that distinguishable particles separate  particle 1 goes one way and particle 2 the other. But indistinguishable particles cannot be separated. And neither one has a distinct path between measurements.
After the particles are measured and become entangled at t_{1}, quantum mechanics describes them with a single twoparticle wave function that is not the product of two oneparticle wave functions. Because electrons are indistinguishable particles, it is not proper to say electron 1 goes this way and electron 2 that way. (Nevertheless, it is convenient to label the particles, as we do in illustrations below.) It is misleading to think that specific particles have distinguishable paths.
Einstein said correctly that at a later time t_{2}, a measurement of one electron's position would instantly establish the position of the other electron  without measuring it explicitly. And this is correct, just as after the collision of two billiard balls, measurement of one ball tells us exactly where the other one is due to conservation of momentum. But this is not "action at a distance." It is more nearly "knowledge at a distance." Note that Einstein used conservation of linear momentum to calculate the position of the second electron. Although conservation laws are rarely cited as the explanation, they are the physical reason that entangled particles always produce correlated results. If the results were not always correlated, the implied violation of a fundamental conservation law would be a much bigger story than mysterious entanglement itself, as interesting as that is.
Einstein criticized the collapse of the wave function as "instantaneousactionatadistance." This criticism resembles the criticisms of Newton's theory of gravitation. Newton's opponents charged that his theory was "action at a distance" and instantaneous. Einstein's own field theory of general relativity shows that gravitational influences travel at the speed of light and are mediated by a gravitational field that shows up as curved spacetime. For Einstein, fields like gravitation and electromagnetism are ponderable, a disturbance of the field at one place is propagated at some finite velocity to other parts of the field. But mathematical probability is not a ponderable field in this sense. When a probability function collapses to unity in one place and zero elsewhere, nothing physical, neither matter nor energy, is moving from one place to the other. Only information changes.
Visualizing Entanglement, Nonlocality, and Nonseparability
Schrödinger said that his "Wave Mechanics" provided more "visualizability" (Anschaulichkeit) than the "damned quantum jumps" of the Copenhagen school, as he called them. He was right. We can use the wave function to visualize EPR.
But we must focus on the probability amplitude wave function of the prepared twoparticle state. We must not attempt to describe the paths or locations of independent particles  at least until after some measurement has been made. We must also keep in mind the conservation laws that Einstein used to describe nonlocal behavior in the first place. Then we can see that the "mystery" of nonlocality for two particles is primarily the same mystery as the singleparticle collapse of the wave function. But there is an extra mystery, one we might call an "enigma," that results from the nonseparability of identical indistinguishable particles. As Richard Feynman said, there is only one mystery in quantum mechanics (the superposition of states, the probabilities of collapse into one state, and the consequent statistical outcomes). The only difference in twoparticle entanglement and nonlocality is that two particles appear simultaneously (in their original interaction frame) when their wave function collapses. We choose to examine a phenomenon which is impossible, absolutely impossible, to explain in any classical way, and which has in it the heart of quantum mechanics. In reality, it contains the only mystery. We cannot make the mystery go away by "explaining" how it works. We will just tell you how it works. In telling you how it works we will have told you about the basic peculiarities of all quantum mechanics. In the time evolution of an entangled twoparticle state according to the Schrödinger equation, we can visualize it  as we visualize the singleparticle wave function  as collapsing when a measurement is made. The discontinuous "jump" is also described as the "reduction of the wave packet." This is apt in the twoparticle case, where the superposition of  +  > and   + > states is "projected" or "reduced" to one of these states, and then further reduced to the product of independent oneparticle states. In the twoparticle case (instead of just one particle making an appearance), when either particle is measured we know instantly those now determinate properties of the other particle that satisfy the conservation laws, including its location equidistant from, but on the opposite side of, the source.
Animation of a twoparticle wave function collapsing  click to restart
Some commentators say that nonlocality and entanglement are a "second revolution" in quantum mechanics, "the greatest mystery in physics," or "science's strangest phenomenon," and that quantum physics has been "reborn." They usually quote Erwin Schrödinger as saying "I consider [entanglement] not as one, but as the characteristic trait of quantum mechanics, the one that enforces its entire departure from classical lines of thought."Schrödinger knew that his twoparticle wave function could not have the same simple interpretation as the single particle, which can be visualized in ordinary 3dimensional configuration space. And he is right that entanglement exhibits a richer form of the "actionatadistance" and nonlocality that Einstein had already identified in the collapse of the single particle wave function. But the main difference is that two particles acquire new properties instead of one, and they do it instantaneously (at faster than light speeds), just as in the case of a singleparticle measurement, where the finite probability of appearing at various distant locations collapses to zero at the instant the particle is found somewhere.
We can enhance our visualization of what might be happening between the time two entangled electrons are emitted with opposite spins and the time one or both electrons are detected. Quantum mechanics describes the state of the two electrons as in a linear combination of  +  > and   + > states. We can visualize the electron moving left to be both spin up  + > and spin down   >. And the electron moving right would be both spin down   > and spin up  + >. We could require that when the left electron is spin up  + >, the right electron must be spin down   >, so that total spin is always conserved. Consider this possible animation of the experiment, which illustrates the assumption that each electron is in a linear combination of up and down spin. It imitates the superposition (or linear combination) with up and down arrows on each electron oscillating quickly. Notice that if you move the animation frame by frame by dragging the dot in the timeline, you will see that total spin = 0 is conserved. When one electron is spin up the other is always spin down.
Since quantum mechanics says we cannot know the spin until it is measured, our best estimate is a 50/50 probability between up and down. This is the same as assuming Schrödinger's Cat is 50/50 alive and dead. But what this means of course is simply that if we do a large number of identical experiments, the statistics for live and dead cats will be approximately 50/50%. We never observe/measure a cat that is both dead and alive! As Einstein noted, QM tells us nothing about individual cats. Quantum mechanics is incomplete in this respect. He is correct, although Bohr and Heisenberg insisted QM is complete, because we cannot know more before we measure, and reality is created (they say) when we do measure. Despite accepting that a particular value of an "observable" can only be known by a measurement (knowledge is an epistemological problem, Einstein asked whether the particle actually (really, ontologically) has a path and position before we measure it? His answer was yes. Here is an animation that illustrates the unprovable assumption that the two electrons are randomly produced in a spinup and a spindown state, and that they remain in those states no matter how far they separate, provided neither interacts until the measurement. An interaction does what is described as decohering the two states.
How Mysterious Is Entanglement?
Some commentators say that nonlocality and entanglement are a "second revolution" in quantum mechanics, "the greatest mystery in physics," or "science's strangest phenomenon," and that quantum physics has been "reborn." They usually quote Erwin Schrödinger as saying
"I consider [entanglement] not as one, but as the characteristic trait of quantum mechanics, the one that enforces its entire departure from classical lines of thought."Schrödinger knew that his twoparticle wave function could not have the same simple interpretation as the single particle, which can be visualized in ordinary 3dimensional configuration space. And he is right that entanglement exhibits a richer form of the "actionatadistance" and nonlocality that Einstein had already identified in the collapse of the single particle wave function. But the main difference is that two particles acquire new properties instead of one, and they do it instantaneously (at faster than light speeds), just as in the case of a singleparticle measurement. Nonlocality and entanglement are thus just another manifestation of Richard Feynman's "only" mystery. In both singleparticle and twoparticle cases paradoxes appear only when we attempt to describe independent particles following a path to measurement by observer A (and/or observer B).
Can a Special Frame Resolve the EPR Paradox?
Is it remotely possible that Einstein deliberately added an asymmetry to a problem that he knew is symmetric, in order to get physicists thinking more seriously about the questions he had been raising for decades, with no one ever taking them. or him, seriously?
Almost every presentation of the EPR paradox begins with something like "Alice observes one particle..." and concludes with the question "How does the second particle get the information needed so that Bob's measurements correlate perfectly with Alice?"
There is a fundamental asymmetry in this framing of the EPR experiment. It is a surprise that Einstein, who was so good at seeing deep symmetries, did not consider how to remove the asymmetry. Consider this reframing: Alice's measurement collapses the twoparticle wave function. The two indistinguishable particles simultaneously appear at locations in a spacelike separation. The frame of reference in which the source of the two entangled particles and the two experimenters are at rest is a special frame in the following sense. As Einstein knew very well, there are frames of reference moving with respect to the laboratory frame of the two observers in which the time order of the events can be reversed. In some moving frames Alice measures first, but in others Bob measures first. If there is a special frame of reference (not a preferred frame in the relativistic sense), surely it is the one in which the origin of the two entangled particles is at rest. Assuming that Alice and Bob are also at rest in this special frame and equidistant from the origin, we arrive at the simple picture in which any measurement that causes the twoparticle wave function to collapse makes both particles appear simultaneously at determinate places with fully correlated properties (just those that are needed to conserve energy, momentum, angular momentum, and spin).
In the twoparticle case (instead of just one particle making an appearance), when either particle is measured, we know instantly those properties of the other particle that satisfy the conservation laws, including its location equidistant from, but on the opposite side of, the source, and its other properties such as spin. We can also ask what happens if Bob is not at the same distance from the origin as Alice. This introduces a positional asymmetry. But there is still no time asymmetry from the point of view of the twoparticle wave function collapse. When Alice detects the particle (with say spin up), at that instant the other particle also becomes determinate (with spin down) at the same distance on the other side of the origin. It now continues, in that determinate state, to Bob's measuring apparatus.
Einstein asked whether the particle has a determinate position(or spin) just before it is measured. Even if it does not, we can say that the electron spin was determined from the moment the twoparticle wave function collapsed. Recall that the twoparticle wave function describing the indistinguishable particles cannot be separated into a product of two singleparticle wave functions. When either particle is measured, they both become determinate.
Why Did Einstein Deemphasize Symmetry and Conservation Principles?
The experiment with two entangled particles was introduced by Einstein in the 1935 EPR paradox paper in the context of conserving momentum. In David Bohm's entangled electrons with total spin zero, the Copenhagen assumption that each particle is in a random unknown combination of spin up and spin down, independent of the other particle, simply because we have not yet measured either particle, is wrong and the source of the “paradox.” Just as a particle has an unknown but definite position, those entangled particles have opposing spins, even if the spins are unknown individually, they are interdependent jointly.
Einstein lived only a few years after Bohm's version and never commented on it as far as we know. But might he have said, following his use of momentum conservation in 1935, and in his 1933 remarks to Leon Rosenfeld, the following. When two particles travel away from the central source, with initial total spin zero, if one is ever measured as spin up, the other must be found with spin down? The operative principle for Einstein here would be conservation of spin. To assume that their spins are independent is to consider the absurd outcome that spins could be found both up (or down), a violation of a conservation principle that is much more egregious than the amazing fact spins are always perfectly correlated in any measurements. Why also did Einstein not say that the overall problem is symmetric. It thus makes no sense to say that one particle is measured first, the other second, if they are in a spacelike separation. In some other moving reference frames it will be the other particle that is measured first. Is Einstein setting a trap for lesser thinkers?
Einstein's Dream of a Continuous Field Theory
Einstein's dream of a continuous and deterministic unified field theory as a "theory of everything" gets in the way of his accepting the nonlocal and nonseparable, indeterministic and asymmetric character of radiation interactions with matter in quantum theory.
Einstein’s main objection to the Copenhagen Interpretation of quantum mechanics was its claim that a particle has no position, or indeed any other observable property, until the particle is measured. He famously told the philosopher Hilary Putnam “Look, I don’t believe that when I am not in my bedroom my bed spreads out all over the room, and whenever I open the door and come in it jumps into the corner.” Despite his reputation as the major critic of quantum mechanics, Einstein came to accept its indeterminism and statistical nature. As we have seen, he had himself discovered these aspects of quantum mechanics. If it is merely constructed on data derived from experience, he said quantum mechanics can only be approximate. Einstein always hoped to discover  or invent  a more fundamental theory, preferably a field theory like the work of Newton and Maxwell and his own relativity theories. He dreamed of a single theory that would unite the gravitational field, the electromagnetic field, the “spinor field,” and even what he called the “ghost field” or “guiding field” of quantum mechanics. Such a theory would use partial differential equations that predict field values continuously for all space and time. That theory would be a free invention of the human mind. Pure thought, he said, could comprehend the real, as the ancients dreamed. Einstein wanted a field theory based on absolute principles such as the constant velocity of light, the conservation laws for energy and momentum, Ehrenfest’s adiabatic principle, symmetry principles, or Boltzmann’s principle that the entropy of a system depends on the possible distributions of its components. We can now see the elements of Einstein’s interpretation, because fields are not substantial, like particles. They are abstract immaterial information that predicts the behavior of a particle at a given point in space and time, should one be there! Fields are information. Particles are information structures. A gravitational field describes paths in curved space that moving particles follow. An electromagnetic field describes the forces felt by an electric charge at each point. The wave function Ψ of quantum mechanics  we can think of it as a possibility field  provides probabilities that a particle will be found at a given point. In all three cases continuous immaterial information describes causal influences over discrete material objects. Note that the local values of all these fields depend on the distribution of matter in the rest of space, the socalled “boundary conditions.” Curvature of space depends on the distribution of masses. Electric fields depend on the distribution of charges. And quantum possibility fields depend on whether there are one or two slits open in the famous and mysterious experiment. The quantum possibility field, calculated from the deterministically evolving Schrödinger equation, is a property of space. Like all fields, it exists whether or not there is a particle present. It only depends on the particle through the particle's wavelength.
Experiments with oneslit and twoslits open, showing the possibilities field calculated from  ψ ^{2}. The possibilities field for two slits open applies whichever slit the particle enters. It is a property of the boundary conditions for the space. Following Einstein's objective reality view that particles have paths even if they cannot be measured, we can now animate the above cases of one slit open or two. Note that with two slits open, the paths start from one slit or the other, distributing themselves randomly between the interference fringes.
We can now summarize Einstein’s thinking about field theories, resulting in a new interpretation of quantum mechanics.
Einstein's Thoughts About Quantum Mechanics
1. Individual particles have the usual classical properties, like position and momentum, plus uniquely quantum properties, like spin, but these properties can only be established statistically. The quantum theory gives us statistical information about an individual particle position, probable values of all possible properties. A particle like an electron is a compact information structure with a definite position and momentum, even if it is unknown.
2. The quantum wave functions are fields. Einstein called them ghost fields or guiding fields. The fields are not the particles. The fields have values in many places at the same time. Particles are at one place at a time. Quantum field values are complex numbers which allow interference effects, causing some places to have no particles. Fields are not localized. Einstein showed that a particle of matter or energy is always localized. Light quanta are emitted and absorbed only as units, for example when one ejects an electron in the photoelectric effect. 3. Because quantum physics does not give us precise information about a particle’s location, it is incomplete when compared to classical physics. Quantum mechanics is a statistical theory and contains only probable information about an individual particle. 4. The Copenhagen notion of complementarity, that a quantum object is both a particle and a wave, or sometimes one and sometimes the other, depending on the measurements performed, is confusing and simply wrong. A particle is always a particle and the wave behavior of its probability field is simply one of the particle’s properties, like its mass, charge, spin, etc. 5. While the probability wave field is abstract and immaterial information, it causally influences the matter or energy, just as the particle’s spin dramatically alters its statistical properties, in particular its allowed positions, as Einstein showed in his 1924 discovery of quantum statistics. These nonintuitive behaviors are simply impossible in classical physics. 6. Although Niels Bohr deserves credit for arranging atoms in the periodic table, the deep reasons for two particles in the first shell and eight in the second were only clear after Einstein discovered spin statistics in 1924, following a suggestion by S. N. Bose. 7. In the twoslit experiment, Einstein’s localized particle always goes through one slit or the other, but when the two slits are open the probability wave function, which influences where the particle can land, is different from the wave function when one slit is open. The possibilities field (a wave) is determined by the boundary conditions of the experiment, which are different when only one slit is open. The particle does not go through both slits. It does not “interfere with itself.” It is never in two places at the same time. 8. The experiment with two entangled particles was introduced by Einstein in the 1935 EPR paradox paper. The Copenhagen assumption that each particle is in a random unknown combination of spin up and spin down, independent of the other particle, simply because we have not yet measured either particle, is wrong and the source of the “paradox.” Just as a particle has an unknown but definite position, entangled particles have definite spins, even if they are unknown individually, they are interdependent jointly. Here is an animation that illustrates the assumption that the two electrons are randomly produced in a spinup and a spindown state, and that they remain in those states no matter how far they separate, provided neither interacts until the measurement. Any interaction does what is described as decohering the two states.
When the particles travel away from the central source, with total spin zero, one is at all times spin up, the other is spin down. The operative principle for Einstein is conservation of spin. To assume that their spins are independent is to consider the absurd outcome that spins could be found both up (or down), a violation of a conservation principle that is much more egregious than the amazing fact spins are always perfectly correlated in any measurements. 9. Erwin Schródinger explained to Einstein in 1936 that two entangled particles share a single wave function that can not be separated into the product of two singleparticle wave functions, at least not until there is an interaction with another system that decoheres their perfect correlation. 10. Einstein ultimately accepted the indeterminism in quantum mechanics and the uncertainty in conjugate variables, despite the clumsy attempt by his colleagues Podolsky and Rosen to challenge uncertainty and restore determinism in the EPR paper. 11. In 1931 Einstein called P.A.M.Dirac’s transformation theory “the most perfect exposition, logically, of this [quantum] theory” even though it lacks “enough information to enable one to decide” a particle’s exact properties. In 1933 Dirac reformulated quantum physics using a Lagrangian rather than the standard Hamiltonian representation. The time integral of the Lagrangian has the dimensions of action, the same as Planck’s quantum of action h. And the principle of least action visualizes the solution of dynamical equations like Hamilton’s as exploring all paths to find that path with minimum action. Dirac’s work led Richard Feynman to invent the pathintegral formulation of quantum mechanics. The transactional interpretations of John Cramer and Ruth Kastner have a similar view. The basic idea of exploring all paths is in many ways equivalent to saying that the probabilities of various paths are determined by a solution of the wave equation using the boundary conditions of the experiment. As we saw above, such solutions involve whether one or two slits are open, leading directly to the predicted interference patterns, given only the wavelength of the particle. 12. In the end, of course, Einstein held out for a continuous field theory, one that could not be established on the basis of any number of empirical facts about measuring particles, but must be based on the discovery of principles, logically simple mathematical conditions which determine the field with differential equations. His lifelong dream was a “unified field theory,” one that at least combined the gravitational field and electromagnetic field, and one that might provide an underpinning for quantum mechanics someday. Einstein was clear that even if his unified field theory was to be deterministic and causal, the statistical indeterminism of quantum mechanics itself would have to be preserved. This seemingly impossible requirement is easily met if we confine the determinism to Einstein’s continuous field theories, which are pure abstract immaterial information. Einstein’s discovery of indeterminism and the statistical nature of physics we apply only to particles, which are information structures, new information in the universe created by the rearrangement of matter, while subject to the second law of thermodynamics.
Summary of Einstein's Objections to Quantum Mechanics
Perhaps the major reason for historians of quantum mechanics (writing since the Copenhagen Interpretation) to largely ignore Einstein is that he was the single most important critic of the quantum mechanics formulated in the late 1920's by Niels Bohr, Werner Heisenberg, Max Born, Pascual Jordan, Wolfgang Pauli, and Paul DIrac, whose work became the "standard orthodox" interpretation of quantum mechanics. So Einstein today is remembered more for his later attacks than for his truly extraordinary fundamental contributions to quantum theory before its socalled "founding.".
Einstein's major objection was that quantum mechanics is a statistical theory, one that predicts probable results for a large number of experiments, but nothing about specific events, like the exact time of a radioactive decay or the direction of spontaneous emission of a photon. This "chance" behavior of individual systems was something that Einstein himself had pointed out in his early papers. But without the ability to predict individual events with certainty, he maintained that quantum mechanics must remain an incomplete theory. Quantum mechanics can precisely specify fewer physical variables than classical mechanics. Because of the indeterminacy principle, only one of each pair of noncommuting observables (momentum or position, for example) can be specified precisely. In this sense, classical theory is more complete. It contains more information. But rather than simply accept Einstein's description and terminology, Bohr, Heisenberg and others engaged in linguistic debates, claiming that quantum theory is itself "complete." They simply denied that more could be known about an underlying reality. A second concern for Einstein was that the wave function ψ for an isolated free particle evolves in time to occupy all space. All positions become equally probable. Yet when we observe the particle, it is always located at some particular place. This does not prove that the particle had a particular place before the observation, but Einstein had a commitment to "elements of reality" that he thought no one could doubt. One of those elements is a particle's position. He asked the question, "Does the particle have a precise position the moment before it is measured?" The Copenhagen answer was sometimes "no," more often it was "we don't know." If there is only one possible prior position for the particle, its path in fourdimensional spacetime is fixed and determinate independently of the time. Complete path information is constant for all time. Quantum theory, by contrast, allows alternative possibilities (with calculable probabilities) that are critical if there is to be more than one possible future. A third (and related) problem for Einstein was the appearance of "nonlocal" behavior, in the "collapse" of the wave function, in the twoslit experiment, and in the EPR experiment "entangling" two particles. Einstein thought in 1927 at the Solvay conference that nonlocality violated his theory of special relativity. He drew a diagram on the blackboard illustrating the problem for a single particle. When the particle appears at point P on the right, what becomes of the wave that was going off to the left? Its "collapse" appears to violate his relativity principle. All the modern collapsedeniers (Bohm, Everett, Zeh, Zurek) are following Einstein and Schrödinger, thinking that the wave function might be something tangible and real. Beyond nonlocality, but closely connected, a fourth problem was the nonseparability of indistinguishable particles. It was the centerpiece of his 1935 criticisms of quantum theory. Already in 1927 Einstein expressed concerns about wave functions that describe two particles. He said that two configurations of a system that are distinguished only by the permutation of two particles of the same species are represented by two different points (in configuration space), which is not in accord with his new results in quantum gas statistics.
For an animated visualization of a "nonlocal" and "nonseparable" twoparticle wave function collapse, see our EPR page.
A twoparticle wave function cannot be the product of independent wave functions for the two components, not even if the partial systems are found to be spatially separated from each other at the moment when they are measured. They had no determinate positions (they were indistinguishable and inseparable) just before the measurements. Einstein thought something must be traveling faster than light speed. That something is only abstract information about probability.
When Einstein published the EPR paper in 1935, it was thirty years since he first had seen the conflict between quantization and relativity. Virtually no other physicists have seen this as clearly as Einstein, and much of the confusion and mystery surrounding entanglement and nonlocality is reduced to the one single mystery (as Richard Feynman described it) of quantum mechanics, the superposition of states and collapse of the wave function, whether a singleparticle or twoparticle wave function!
A fifth difficulty arose from Einstein's deep belief that any physical theory must be based on a continuous field. For Einstein, physical objects must be described by continuous functions of field variables in fourdimensional spacetime coordinates. In quantum field theory (QFT), particles are functions of (singularities in) these fields. In quantum electrodynamics (QED), fields are merely properties of aggregated particles. Which then are the more fundamental?
Heisenberg and Bohr did not require a "conscious observer" to collapse the wave function in a measurement, but only the connection to the observer's mind for the results of an experiment to become human knowledge.
A sixth objection was the "Copenhagen interpretation" of the measurement process as requiring a conscious "observer" to produce "collapses" of the wave function. Einstein thought it absurd that his bed would diffuse throughout his bedroom until the moment that he opened the door and looked at it. It is not human observation that collapses wave functions, but any interaction of one quantum system with another. Focusing on information created or destroyed in particle interactions solves the famous "measurement problem."
A related objection was Bohr's philosophical commitment to "complementarity," which Einstein compared to Kant's dualistic subjectiveobjective and phenomenalnoumenal thinking. Einstein said he could not understand complementarity "despite much effort which I have expended on it." Rather than directly answer, indeed accept, Einstein's claims that quantum theory is statistical and therefore incomplete, Bohr amateurishly philosophized about "complementary" classical and quantum realities. There is only one quantum reality, which converges in the limit of large numbers of particles (whether radiation or matter) to appear "classical" and adequately determined for most practical purposes. To summarize, Einstein disagreed initially with the fundamental indeterminism and statistical character of quantum theory. Inspired by his Spinozan deterministic theory of nature, Einstein repeatedly asserted that "God does not play dice." Ironically, it was Einstein himself who first clearly identified quantumlevel indeterminism (over a decade before Heisenberg's discovery of uncertainty and acausality). Einstein saw that the decay time of a radioactive nucleus and the direction of a spontaneously emitted photon are nothing but the consequence of "chance" (Zufall) in quantum theory. On the other hand, his determinism did not prevent Einstein from saying that physical concepts and the laws of nature are "free creations of the human mind." Einstein's magnificent contributions to quantum theory are not only such "free creations," but "chance" is half of the best explanation for the existence of human creativity and freedom of the will from predeterminism. The adequate determinism of macroscopic structures (like human beings) is the other half of the twostage model of free will.
Brief Review of the Chronology
Although it was Max Planck who introduced the notion of quantization (in 1900) to develop his blackbody radiation law, Planck did not believe for many years that radiation itself was quantized. It was Einstein who introduced the light quantum hypothesis, in 1905. Planck did not accept Einstein's light quanta for several years. He said in the discussion period following Einstein's 1909 paper, "That seems to me to be a step that, in my opinion, is not yet called for." Bohr opposed light quanta for two decades after Einstein's hypothesis, and rarely gave him much credit thereafter. In 1913, Neils Bohr's "old quantum theory" introduced stationary eigenstates in his "Bohr atom," but he continued to believe that the radiation emitted in "quantum jumps" between those states is continuous and classical until the middle 1920's. Bohr postulated that the radiation emitted or absorbed was given by the formula E = hν, but it was Planck who first proposed this relation and Einstein who derived (proved) this result (in 1916). Bohr did not accept the reality of light quanta (photons) until after the failure of his BohrKramersSlater attempt to combine discontinuous electron jumps with continuous radiation emission in 1924. As early as 1921, Einstein spoke to several colleagues about the wave as an immaterial "ghost field" (Gespensterfeld) that predicts the probability of finding his light quanta and as a leading or pilot field (Führungsfeld) that guides the paths of the energy quanta. In 1924, Louis deBroglie predicted the wave theory of matter. It was based on Einstein's writings on waveparticle duality fifteen years earlier and perhaps on Einstein's speculations about a pilot field. Einstein was an enthusiastic supporter of deBroglie's wave theory. It brought the symmetry and equivalence between matter and radiation that Einstein asked for in his earliest works. In 1926, Erwin Schrödinger developed his wave equation and "wave mechanics," which he showed could produce exactly the same results as HeisenbergJordanBorn "matrix mechanics" (and considerably simplify calculations, to Heisenberg's embarrassment). Schrödinger said he was inspired by Einstein's "short but infinitely farseeing remarks" into the wave and particle theories of radiation. Also in 1926, Max Born offered his "statistical interpretation" of the wave function for a scattered particle. Einstein's picture of the quantum theory of radiation had interpreted the wave picture as the density of the statistical distribution of photons. Following the Einstein precedent that waves predicted the probabilities or number of light quanta (later photons), Born described deBroglieSchrödinger matter waves as predicting the probabilities for different paths in atom and electron collision processes. Few commentators, give Einstein credit for the statistical interpretation, presumably because Einstein was so critical of it. Born himself wrote Einstein, that he got "my idea, to conceive of the Schrödinger wave field as a ghost field in your sense," viz., Einstein's "Gespensterfeld". For Einstein, Born's work on material particles (which mirrored Einstein's own light quanta insights) confirmed quantum theory as an incomplete statistical theory. Schrödinger violently disagreed with Born's statistical view. He even denied the reality of "quantum jumps," as did later followers of Einstein and Schrödinger like David Bohm, John Wheeler, John Bell, Hugh Everett, H. Dieter Zeh, Wojciech Zurek, and many other "collapsedeniers" to this day. In 1927, Werner Heisenberg announced his indeterminacy principle and claimed that nature was acausal. But Einstein first found that chance was the only possible explanation for the spontaneous emission of radiation and the spontaneous decay of radioactive nuclei (again in 1916). Einstein saw acausality in nature a decade before Heisenberg. To be sure, such "chance" bothered Einstein. He called it a "weakness in the theory." But he still deserves some credit for seeing the discrete, discontinuous, and acausal nature of quantum physics long before those who do get the credit. At the Solvay conference in 1927, Bohr and Heisenberg claimed that Einstein suggested a number of thought experiments to disprove Heisenberg's indeterminacy principle. Heisenberg said that Bohr defended the principle successfully again and again. And at Solvay Einstein made perfectly clear his concern that fasterthanlight effects might be involved as the probability wave of quantum mechanics collapsed instantly when the particle is discovered at a particular location. Did Einstein already see this as early as 1905 (when he enunciated his principle of relativity)? There he wondered how energy in a light wave spread out into a large volume of space could get itself all together again to be absorbed by another atom. Eight years later, Einstein made his most famous attack on the statistical and incomplete nature of quantum mechanics with two Princeton colleagues, Boris Podolsky and Nathan Rosen. The EinsteinPodolskyRosen paper, and a Schrödinger paper (on his famous cat) the same year, made famous the concepts of "nonlocality," "nonseparability," and "entanglement" that are so popular today with some scientists and many philosophers of science who dislike the irreducible statistical and indeterministic aspects of quantum theory.
Born gives Einstein Credit for the Statistical Interpretation
I had therefore been at pains, as early as the end of 1925, to extend the matrix method, which obviously covered only oscillatory processes, in such a way as to be applicable to aperiodic processes. I was at that time the guest of the Massachusetts Institute of Technology in the U.S.A., and there I found in NORBERT WIENER a distinguished collaborator. In our joint paper [16] we replaced the matrix by the general concept of an operator and, in this way, made possible the description of aperiodic processes. Yet we missed the true approach, which was reserved for SCHRÖDINGER; and I immediately took up his method, since it promised to lead to an interpretation of the ψfunction. Once more an idea of EINSTEIN'S gave the lead. He had sought to make the duality of particles (light quanta or photons) and waves comprehensible by interpreting the square of the optical wave amplitudes as probability density for the occurrence of photons. This idea could at once be extended to the ψfunction: the idea of electron waves was familiar to me when Schrödinger's papers on the structure of simple atoms appeared. At that time it was clear that the proper interpretation of quantum mechanics must be of a statistical type. There were several attempts to formulate this, all based on matrix mechanics, by Heisenberg, Bohr, Kramers, and others. I do not remember when and how the idea struck me that collision processes, i.e. aperiodic motions, must provide the clue for the solution; for the relative numbers of the incoming and outgoing particles could be counted and regarded as empirical probability values. I think this must have been already in my mind when I was at M.I.T. and tried, together with Norbert Wiener, to find a formulation of quantum mechanics for aperiodic motions. As soon as I had digested Schrödinger's papers I saw the right way to approach this, guided by a remark of Einstein's about the meaning of intensity of light (i.e. of an electromagnetic wave) in terms of photons: this intensity must represent the number of photons; but the latter was of course to be understood statistically, as the average over a certain photon distribution. Einstein had considered in depth the statistical nature of this distribution, particularly the fluctuations about the mean, which are closely connected with Planck's radiation formula. These investigations were well known to me, and they led immediately to the conjecture that the intensity of the de Broglie wave, i.e. the (absolute) square of Schrödinger's wave function, must be regarded as the probability density, which is the probability of finding a particle in a unit of volume.
Details from Einstein's 19051935 Papers
Long before the best known arguments for quantum mechanics by Heisenberg, Born, Jordan and others in the late nineteentwenties, Einstein had followed Max Planck's postulate of a "quantum of action" (for Planck this was just a mathematical device applied to hypothetical resonant oscillators needed to derive his radiation law) to the conclusion that electromagnetic radiation consists of discrete particles of light (Einstein called them "lichtquant") that are emitted and absorbed as indivisible units. As matter is composed of atomic units, Einstein argued that energy itself is also quantized and can be emitted and absorbed only in whole units. He described his light quantum hypothesis in 1905:
On the modern quantum view, what spreads out is a wave of probability amplitude ψ for absorbing a whole photon somewhere. Einstein may be already concerned that an energy quantum spread out over space could not instantly collect itself in one place (to be absorbed by another atom) without traveling faster than the speed of light
In accordance with the assumption to be considered here, the energy of a light ray spreading out from a point source is not continuously distributed over an increasing space but consists of a finite number of energy quanta which are localized at points in space, which move without dividing, and which can only be produced and absorbed as whole units.Planck in 1900 explained the spectral distribution of colors (wavelengths) in blackbody electromagnetic radiation by using Boltzmann’s principle that the entropy S of a gas is related to the probabilities W for random distribution of molecules in different places in its container (S = k logW, where k is Boltzmann’s constant). Boltzmann’s calculations of probabilities used the number of ways that particles can be distributed in various volumes of space. Planck used the same combinatorial analysis, but now for the number of ways that discrete elements of energy could be distributed among a number of radiation oscillators. To simplify calculations, both Boltzmann and Planck assumed that energies (for matter) could be considered multiples of a unit of energy, E = ε, 2ε, 3ε ... Plank regarded this quantum hypothesis as a mathematically convenient device, but not necessarily representing reality. He found the density of radiation with frequency ν to be
ρ_{ν} = (8πhν^{3}/c^{3}) / (e^{hν/kT}  1). Planck's "blackbody" radiation law was the first known connection between the mechanical laws of matter and the laws of electromagnetic energy. Planck realized that he had made a great step in physical understanding, "the greatest discovery in physics since Newton," he reportedly told his sevenyearold son in 1900. In particular, Planck found that Boltzmann's statistical mechanics constant k = R/N, derived from the distribution of velocities of material gas particles, appears in his new law for the distribution of electromagnetic radiation energy. Planck established an independent and very accurate value for Boltzmann's constant (he gave it the symbol k). His blackbody radiation distribution law of course also includes the new Planck constant h (the "quantum of action"). Planck also found a value for Avogadro's number of molecules in a mole (gram molecular weight) of a gas. This experimental agreement greatly impressed Einstein. Einstein was impressed with the experimental accuracy of the Planck radiation law. But beyond that, Einstein was very interested in the interaction between radiation and matter that Planck had now probed. Five years later, Einstein published three famous papers, all exploring the interaction between radiation and matter. He showed that there are fundamental similarities between light and material particles. Best known is his theory of special relativity (connecting energy and matter  as did Planck  but now with the famous equation E = mc^{2}), his theory of Brownian motion, and his explanation of the photoelectric effect (for which he was awarded the Nobel Prize). But in this third paper, Einstein proposed that electromagnetic radiation really consists of discrete quantities of light (he called them lichtquant, light quanta, today they are called photons). Einstein added physical significance to Planck's equation for radiant energy, E = hν, where h is Planck’s constant and ν is the frequency of the radiation. Einstein also derived the blackbody radiation law. His assumptions were more physical, where Planck's were heuristic guesses chosen to fit the data. And Einstein saw the profound physical implications of assuming that both matter and radiation come in discrete particles or quanta (an idea that Einstein pointed out went back to Newton, before Maxwell's theory of electromagnetism introduced the concept of continuous fields  which Einstein made the basis of all his future work in general relativity). Boltzmann had made the laws of physics merely statistical laws. Where Planck did not accept the reality of quanta until some years after Einstein's work, Einstein was alone among physicists believing in the reality of light quanta and, at least in his early work, believing in the statistical nature of physics, even if he decried it as a "weakness in the theory." When in 1913 Neils Bohr published his work on the quantization of energy levels in atoms (the socalled "old" quantum theory), he did not imagine that the discrete transitions  "quantum jumps"  between energy levels involved quantized light particles. Bohr thought the electron jumps between "orbits" were quantum and discontinuous, but he thought the radiation emitted was discrete, E_{m}  E_{n}= hν, a classical and continuous wave going out in all directions. In 1909, Einstein speculated about the connection between wave and particle views:
As late as 1917, Einstein felt very much alone in believing the reality (his emphasis) of light quanta: I do not doubt anymore the reality of radiation quanta, although I still stand quite alone in this conviction Einstein in 1916 had just derived his A and B coefficients describing the absorption, spontaneous emission, and (his newly predicted) stimulated emission of radiation. In two papers, "Emission and Absorption of Radiation in Quantum Theory," and "On the Quantum Theory of Radiation," he derived the Planck law (for Planck it was mostly a guess at the formula), he derived Planck's postulate E = hν, and he derived Bohr's second postulate E_{m}  E_{n} = hν. Einstein did this by exploiting the obvious relationship between the MaxwellBoltzmann distribution of gas particle velocities and the distribution of radiation in Planck's law. The formal similarity between the chromatic distribution curve for thermal radiation and the Maxwell velocitydistribution law is too striking to have remained hidden for long. In fact, it was this similarity which led W. Wien, some time ago, to an extension of the radiation formula in his important theoretical paper, in which he derived his displacement law...Not long ago I discovered a derivation of Planck's formula whichFnote that was closely related to Wien's original argument and which was based on the fundamental assumption of quantum theory. This derivation displays the relationship between Maxwell's curve and the chromatic distribution curve and deserves attention not only because of its simplicity, but especially because it seems to throw some light on the mechanism of emission and absorption of radiation by matter, a process which is still obscure to us.But the introduction of MaxwellBoltzmann statistical mechanical thinking to electromagnetic theory has produced what Einstein called a "weakness in the theory." It introduces the reality of an irreducible objective chance! If light quanta are particles with energy E = hν traveling at the velocity of light c, then they should have a momentum p = E/c = hν/c. When light is absorbed by material particles, this momentum will clearly be transferred to the particle. But when light is emitted by an atom or molecule, a problem appears.
The "statistical interpretation" of Max Born tells us the outgoing wave is the probability amplitude wave function Ψ, whose absolute square is the probability of finding a light particle in an arbitrary direction.
Conservation of momentum requires that the momentum of the emitted particle will cause an atom to recoil with momentum hν/c in the opposite direction. However, the standard theory of spontaneous emission of radiation is that it produces a spherical wave going out in all directions. A spherically symmetric wave has no preferred direction. In which direction does the atom recoil? Einstein asked:
Does the molecule receive an impulse when it absorbs or emits the energy ε? For example, let us look at emission from the point of view of classical electrodynamics. When a body emits the radiation ε it suffers a recoil (momentum) ε/c if the entire amount of radiation energy is emitted in the same direction. If, however, the emission is a spatially symmetric process, e.g., a spherical wave, no recoil at all occurs. This alternative also plays a role in the quantum theory of radiation. When a molecule absorbs or emits the energy ε in the form of radiation during the transition between quantum theoretically possible states, then this elementary process can be viewed either as a completely or partially directed one in space, or also as a symmetrical (nondirected) one. It turns out that we arrive at a theory that is free of contradictions, only if we interpret those elementary processes as completely directed processes. An outgoing light particle must impart momentum hν/c to the atom or molecule, but the direction of the momentum can not be predicted! Neither can the theory predict the time when the light quantum will be emitted. Einstein called this weakness by its German name  Zufall (chance). Such a random time was not unknown to physics. When Ernest Rutherford derived the law for radioactive decay of unstable atomic nuclei in 1900, he could only give the probability of decay time. Einstein saw the connection with radiation emission: It speaks in favor of the theory that the statistical law assumed for [spontaneous] emission is nothing but the Rutherford law of radioactive decay.But the inability to predict both the time and direction of light particle emissions, said Einstein in 1917, is "a weakness in the theory..., that it leaves time and direction of elementary processes to chance (Zufall, ibid.)." It is only a weakness for Einstein, of course, because his God does not play dice. Einstein clearly saw, as none of his contemporaries did, that since spontaneous emission is a statistical process, it cannot possibly be described with classical physics. The properties of elementary processes required...make it seem almost inevitable to formulate a truly quantized theory of radiation. Einstein may not have liked this conceptual crisis, but his insights into the indeterminism involved in quantizing matter and energy were known, if largely ignored, over a decade before Heisenberg's quantum theory introduced his famous uncertainty principle in 1927. Heisenberg states that the exact position and momentum of an atomic particle can only be known within certain (sic) limits. The product of the position error and the momentum error is greater than or equal to Planck's constant h/2π.
ΔpΔx ≥ h/2π
Indeterminacy (Unbestimmtheit) was Heisenberg's original name for his principle. It is a better name than the more popular uncertainty, which connotes lack of knowledge. Quantum indeterminacy is ontological as well as epistemic lack of information. Heisenberg declared that the new quantum theory disproved causality with facts that were first described by Einstein years earlier. He did not reference Einstein's 1916 work on the breakdown of causality. Heisenberg simply says: We cannot  and here is where the causal law breaks down  explain why a particular atom will decay at one moment and not the next, or what causes it to emit an electron in this direction rather than that. Heisenberg (and Bohr) were not convinced about Einstein's light quanta as late as 1926! Whether or not I should believe in light quanta, I cannot say at this stage. Radiation quite obviously involves the discontinuous elements to which you refer as light quanta. On the other hand, there is a continuous element, which appears, for instance, in interference phenomena, and which is much more simply described by the wave theory of light. But you are of course quite right to ask whether quantum mechanics has anything new to say on these terribly difficult problems. I believe that we may at least hope that it will one day. It is important to note that Einstein's indeterminism of time and direction is an intrinsic property of the interaction of radiation with matter. It does not depend on limits put on measurements, as Heisenberg's "uncertainty" suggests, nor on the presence of a conscious observer, as Bohr's Copenhagen interpretation seems to imply. Where Bohr and Heisenberg describe epistemic limits to knowledge, Einstein's light quanta shows us an ontologically indeterministic world, independent of any observation or measurement. Einstein says: If the molecule suffers a loss of energy in the amount of hν without external stimulation, i.e., by emitting the energy in the form of radiation (spontaneous emission), then this process too is a directional one. There is no emission of radiation in the form of spherical waves. The molecule suffers a recoil in the amount of hν/c during this elementary process of emission of radiation; the direction of the recoil is, at the present state of theory, determined by "chance"... Although Einstein initially was a strong critic of quantum theory and its implications for indeterminism and a statistical nature of reality, from the 1930's on he never said that quantum mechanics is "incorrect"  as far as it goes  only that something else would likely be added to quantum physics in the future, making it "complete."
Above all, however, the reader should be convinced that I fully recognize the very important progress which the statistical quantum theory has brought to theoretical physics. As early as 1930, Einstein marveled at the logical strength of the quantum theory, especially its formulation by Paul Dirac, "to whom, in my opinion, we owe the most perfect exposition, logically, of this [quantum] theory." Note that Einstein's views about quantum mechanics in 1949 were essentially unchanged from his views in 1930, and his basic concerns about particles acting like waves and thus violating his theory of relativity go back to 1909 or even 1905. See Einstein's explanation of how continuous field theories came to be a part of our description of reality  alongside material particles  as a result of Maxwell's equations  in the 1931 article "Maxwell's Influence on the Evolution of the Idea of Physical Reality." Einstein in his later years grew pessimistic about the possibilities for deterministic continuous field theories, by comparison with indeterministic and statistical discontinuous particle theories like those of quantum mechanics. To Leopold Infeld he wrote in 1941, "I tend more and more to the opinion that one cannot come further with a continuum theory."In his 1949 autobiography (he called it his obituary) for his Schilpp volume he wrote an extensive analysis of his criticism of the quantum theory, repeating the concerns he had first developed in 1935. It is worth looking at them completely here. I must take a stand with reference to the most successful physical theory of our period, viz., the statistical quantum theory which, about twentyfive years ago, took on a consistent logical form (Schrödinger, Heisenberg, Dirac, Born). This is the only theory at present which permits a unitary grasp of experiences concerning the quantum character of micromechanical events. This theory, on the one hand, and the theory of relativity on the other, are both considered correct in a certain sense, although their combination has resisted all efforts up to now. This is probably the reason why among contemporary theoretical physicists there exist entirely differing opinions concerning the question as to how the theoretical foundation of the physics of the future will appear. Einstein wrote his friend Michele Besso in 1954 to express his lost hopes for a continuous field theory like that of electromagnetism or gravitation, "I consider it quite possible that physics cannot be based on the field concept, i.e:, on continuous structures. In that case, nothing remains of my entire castle in the air, gravitation theory included, [and of] the rest of modern physics." The fifth edition of The Meaning of Relativity included a new appendix on Einstein's field theory of gravitation. In the final paragraphs of this work, his last, published posthumously in 1956, Einstein wrote: Is it conceivable that a field theory permits one to understand the atomistic and quantum structure of reality ? Almost everybody will answer this question with "no"...
Einstein Papers on Quantum Theory
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"On the Method of Theoretical Physics," The Herbert Spencer Lecture, Oxford, June 10, 1933, Ideas and Opinions, Albert Einstein, Bonanza Books, 1954, pp.270276; original in Mein Weltbild, Amsterdam, 1934, (PDF)
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For Teachers
What Einstein Really Wanted
What Einstein Disliked, But Understood Might Be The Case
Critical Einstein Quantum Ideas
The Comprensibility of the Universe
I learned as a young physics student this wonderful quotation of Einstein that I repeated to my students for many years.
"The most incomprehensible thing about the universe is that it is comprehensible." It has therefore been disturbing in recent years to find versions that eliminate Einstein's beautiful symmetry, or asymmetry, or perhaps even antisymmetry?, with respect to comprehensibility. Many have no doubt been guided by the version in Alice Calaprice's definitive collection of quotations, taken from the English translation of Einstein's essay "Physik und Realität," originally published in German by the Journal of the Franklin Institute in 1936, then translated and republished in 1954 as "Physics and Reality," for Einstein's book "Ideas and Opinions". “the eternal mystery of the world is its comprehensibility...the fact that it is comprehensible is a miracle."Calaprice describes it as 'popularly rephrased as' "The most incomprehensible thing about the universe is that it is comprehensible." Einstein's original German version "Physik und Realität," shows that Einstein himself used the more poetic and rhetorically strong antisymmetric words Unbegreifliche and Begreiflichkeit, i.e., incomprehensible and comprehensibility, n.b., an adjective and a noun. And it shows that Caprice's version is a composite elided (...) from two different sentences in Einstein's text, one mistranslating "ewig Unbegreiflich" as "eternal mystery," the other properly translating "ein Wunder" as "a miracle." "Man kann sagen: Das ewig Unbegreifliche an der Welt ist ihre Begreiflichkeit." (Einstein's antisymmetry is clear here) We can note that a better (e.g., Google) translation for Einstein's original words would be. "The eternally incomprehensible (thing) about the world is its comprehensibility." For Scholars
References
Guido Bacciagaluppi
John S. Bell
Don Howard
Martin J. Klein Thomas S. Kuhn
Hendrik A. Kramers
Hendrik Lorentz
Jagdish Mehra
Abraham Pais
John Stachel
Einstein's General Relativity
Einstein argued that all physical measurements are simply "coincidences" between material or energetic quanta (essentially particles) and the measuring devices, material sticks (rulers) and clocks. The measurements or "observations" give us quantitative information about spatial relations between events in spacetime (spacetime coincidences).
The continuous threedimensional spatial geometry and continuous time dimension provide a four dimensional "system of reference" that "facilitates our description" of these coincidences. That this requirement of general covariance, which takes away from space and time the last remnant of physical objectivity, is a natural one, will be seen from the following reflexion. All our spacetime verifications invariably amount to a determination of spacetime coincidences. If, for example, events consisted merely in the motion of material points, then ultimately nothing would be observable but the meetings of two or more of these points. Moreover, the results of our measurings are nothing but verifications of such meetings of the material points of our measuring insmments with other material points, coincidences between the hands of a clock and points on the clock dial, and observed pointevents happening at the same place and the same time. For Teachers
For Scholars
