Citation for this page in APA citation style.           Close


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 Belsham
Henri Bergson
George Berkeley
Isaiah Berlin
Richard J. Bernstein
Bernard Berofsky
Robert Bishop
Max Black
Susanne Bobzien
Emil du Bois-Reymond
Hilary Bok
Laurence BonJour
George Boole
Émile Boutroux
F.H.Bradley
C.D.Broad
Michael Burke
C.A.Campbell
Joseph Keim Campbell
Rudolf Carnap
Carneades
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
Herbert Feigl
John Martin Fischer
Owen Flanagan
Luciano Floridi
Philippa Foot
Alfred Fouilleé
Harry Frankfurt
Richard L. Franklin
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
William James
Lord Kames
Robert Kane
Immanuel Kant
Tomis Kapitan
Jaegwon Kim
William King
Hilary Kornblith
Christine Korsgaard
Saul Kripke
Andrea Lavazza
Keith Lehrer
Gottfried Leibniz
Leucippus
Michael Levin
George Henry Lewes
C.I.Lewis
David Lewis
Peter Lipton
C. Lloyd Morgan
John Locke
Michael Lockwood
E. Jonathan Lowe
John R. Lucas
Lucretius
Alasdair MacIntyre
Ruth Barcan Marcus
James Martineau
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
Friedrich Nietzsche
John Norton
P.H.Nowell-Smith
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
Jean-Paul Sartre
Kenneth Sayre
T.M.Scanlon
Moritz Schlick
Arthur Schopenhauer
John Searle
Wilfrid Sellars
Alan Sidelle
Ted Sider
Henry Sidgwick
Walter Sinnott-Armstrong
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
William Whewell
Alfred North Whitehead
David Widerker
David Wiggins
Bernard Williams
Timothy Williamson
Ludwig Wittgenstein
Susan Wolf

Scientists

Michael Arbib
Bernard Baars
Gregory Bateson
John S. Bell
Charles Bennett
Ludwig von Bertalanffy
Susan Blackmore
Margaret Boden
David Bohm
Niels Bohr
Ludwig Boltzmann
Emile Borel
Max Born
Satyendra Nath Bose
Walther Bothe
Hans Briegel
Leon Brillouin
Stephen Brush
Henry Thomas Buckle
S. H. Burbury
Donald Campbell
Anthony Cashmore
Eric Chaisson
Jean-Pierre Changeux
Arthur Holly Compton
John Conway
John Cramer
E. P. Culverwell
Charles Darwin
Terrence Deacon
Louis de Broglie
Max Delbrück
Abraham de Moivre
Paul Dirac
Hans Driesch
John Eccles
Arthur Stanley Eddington
Paul Ehrenfest
Albert Einstein
Hugh Everett, III
Franz Exner
Richard Feynman
R. A. Fisher
Joseph Fourier
Lila Gatlin
Michael Gazzaniga
GianCarlo Ghirardi
J. Willard Gibbs
Nicolas Gisin
Paul Glimcher
Thomas Gold
A.O.Gomes
Brian Goodwin
Joshua Greene
Jacques Hadamard
Patrick Haggard
Stuart Hameroff
Augustin Hamon
Sam Harris
Hyman Hartman
John-Dylan Haynes
Martin Heisenberg
Werner Heisenberg
John Herschel
Jesper Hoffmeyer
E. T. Jaynes
William Stanley Jevons
Roman Jakobson
Pascual Jordan
Ruth E. Kastner
Stuart Kauffman
Martin J. Klein
Simon Kochen
Stephen Kosslyn
Ladislav Kovàč
Rolf Landauer
Alfred Landé
Pierre-Simon Laplace
David Layzer
Benjamin Libet
Seth Lloyd
Hendrik Lorentz
Josef Loschmidt
Ernst Mach
Donald MacKay
Henry Margenau
James Clerk Maxwell
Ernst Mayr
Ulrich Mohrhoff
Jacques Monod
Emmy Noether
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
Adolphe Quételet
Juan Roederer
Jerome Rothstein
David Ruelle
Erwin Schrödinger
Aaron Schurger
Claude Shannon
David Shiang
Herbert Simon
Dean Keith Simonton
B. F. Skinner
Roger Sperry
John Stachel
Henry Stapp
Tom Stonier
Antoine Suarez
Leo Szilard
William Thomson (Kelvin)
Peter Tse
Heinz von Foerster
John von Neumann
John B. Watson
Daniel Wegner
Steven Weinberg
Paul A. Weiss
John Wheeler
Wilhelm Wien
Norbert Wiener
Eugene Wigner
E. O. Wilson
H. Dieter Zeh
Ernst Zermelo
Wojciech Zurek

Presentations

Biosemiotics
Free Will
Mental Causation
James Symposium
 
Complementarity
In the late Winter of 1927, Neils Bohr went skiing for a few weeks in Norway, during which he analyzed the puzzling situation in quantum mechanics in deeply philosophical terms.

In the previous two years, Max Born, with his clever students Werner Heisenberg and Pascual Jordan, had developed the quantum mechanics of material particles. They had derived most of the results of Bohr's old quantum theory, eliminating his idea of semi-classical orbits but confirming Bohr's "quantum postulate of stationary states with electrons "jumping" between them, radiating energy with E2 - E1 = hν, following Max Planck's hypothesis about the quantum of action.

And just the year before, Erwin Schrödinger developed an alternative "wave mechanics," which he showed gives exactly the same results as quantum mechanics, but without some of the major assumptions in Bohr's earlier work, which had been adopted also by Heisenberg. In his 1929 textbook, Heisenberg dubbed their work "Der Kopenhagener Geist," many years later known as the "Copenhagen interpretation" of quantum mechanics. Where Bohr and Heisenberg described the stationary states with arbitrary quantum numbers, Schrödinger showed quantum numbers emerge naturally from the number of nodes in his wave function that could fit around an electron orbit (an idea that Louis de Broglie had proposed earlier).

The dualistic view that matter might consist of either particles or waves (or maybe both) must surely have inspired Bohr to think about complementary relations, but there are strong reasons to think that he might not have wanted to identify his complementarity with Einstein's ideas about "wave-particle duality".

Heisenberg said that "The main point was that Bohr wanted to take this dualism between waves and corpuscles as the central point of the problem." But Bohr also used the term complementary to describe the "reciprocal uncertainty" between momentum and position in Heisenberg's indeterminacy relations. Bohr said:

the measurement of the positional coordinates of a particle is accompanied not only by a finite change in the dynamical variables, but also the fixation of its position means a complete rupture in the causal description of its dynamical behaviour, while the determination of its momentum always implies a gap in the knowledge of its spatial propagation. Just this situation brings out most strikingly the complementary character of the description of atomic phenomena [italics added]

Bohr may never have completely accepted Albert Einstein's idea that light itself might consist of particles, since quantum particles are complements of classical waves. In 1905, Einstein had proposed his "light-quantum hypothesis," that light came in discrete and discontinuous quantities, something like Newton's "light corpuscles."

Einstein wrote in 1905:

On the modern quantum view, what spreads out is a wave of probability amplitude for absorbing a whole "light quantum" somewhere. The wave function ψ should be thought of as a "possibility" function
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.

Bohr resisted Einstein's "light-quantum hypothesis" in 1913. His Bohr model of the atom postulated that there are "stationary states" with energy levels En. His second postulate was that electrons jump discontinuously between levels, emitting or absorbing radiation of frequency ν, where

Em - En = hν

As obvious as it is today that Bohr's is a "photon" (as it was dubbed in the middle 1920's), Bohr thought that the radiation emitted or absorbed was continuous and classical electromagnetism. It is not clear that Bohr had completely accepted photons and the dual nature of light even as he formulated his philosophical notion of complementarity in his "Como Lecture" of 1927. He seems to have accepted it in 1949, in his tribute to Einstein.

Einstein had written as early as 1909 that the wave theory of light might need to be augmented to explain his particle-like properties.

This was the beginning of wave-particle duality that Bohr would reconcile
with the idea of complementarity in quantum mechanics
When light was shown to exhibit interference and diffraction, it seemed almost certain that light should be considered a wave...A large body of facts shows undeniably that light has certain fundamental properties that are better explained by Newton's emission theory of light than by the oscillation theory. For this reason, I believe that the next phase in the development of theoretical physics will bring us a theory of light that can be considered a fusion of the oscillation and emission theories...

When Bohr returned from his skiing vacation, he received a draft paper from Heisenberg claiming that some physical variables might be measured precisely, but then their canonically conjugate variables would have a very large error. This is his famous "indeterminacy principle." If a momentum measurement has accuracy Δp and position accuracy Δx than the product of the two indeterminacies is Δp Δx ≥ h, where h is Planck's constant for the quantum of action.

Bohr asked Heisenberg to include his notion of complementarity, and perhaps his derivation of indeterminacy from pure wave-mechanical considerations, in his new paper. This upset Heisenberg greatly, because he thought that Schrödinger's "wave mechanics" added nothing to his particle-oriented "matrix mechanics." Bohr thought both were needed. Though somewhat contradictory, they were his first example of "complementarity."

Definitions of complementarity today almost always include wave-particle duality, but Bohr was so vague about the precise meaning of his term complementarity when he introduced it in his 1927 "Como Lecture" that it is confusing to this day. One thing he did in the Como Lecture was to argue that both Heisenberg's discontinuous and indeterministic particle picture and Schrödinger's continuous and deterministic wave picture were both needed in quantum mechanics. The theories themselves, matrix mechanics and wave mechanics, are "complementary."

Almost no one, least of all Bohr, gave credit to Einstein, for his 1909 insight that both wave and particle pictures needed to be fused, or to his views in the early 1920's that the wave was a "Gespensterfeld" (ghost field) that guides the particles. Ironically, and unjustly, to this day the "Bohr atom" is taught as discontinuous "jumps" between energy levels accompanied by the emission or absorption of a photon, whereas Bohr fought against Einstein's light quantum hypothesis for decades. Einstein developed the quantum theory of radiation, explaining emission, absorption, and the radical hypothesis of "stimulated emission" (that led to the invention of the laser) in 1916! But it is Bohr's name most often cited.

Bohr claimed that an experimental apparatus must always be treated as a classical object and described using ordinary language. He thought that specific experiments could reveal only part of the quantum nature of microscopic objects. For example, one experiment might reveal a particle's dynamical properties such as energy, momentum, position, etc. Another experiment might reveal wavelike properties. But no one experiment could exhaustively reveal both. The experiments needed to reveal both are "complementary."

Bohr's first definition of complementarity in the Como lecture somewhat opaquely contrasts the "space-time coordination" with the "claim of causality."

Space-time co-ordination and the claim of causality are complementary.

They "symbolize" observation
and definition,
also complementary?

Relativity has a limit
v / c → 0.

Quantum mechanics
has the limit h → 0
(better h / m → 0).

The very nature of the quantum theory thus forces us to regard the space-time co-ordination and the claim of causality, the union of which characterises the classical theories, as complementary but exclusive features of the description, symbolising the idealisation of observation and definition respectively. Just as the relativity theory has taught us that the convenience of distinguishing sharply between space and time rests solely on the smallness of the velocities ordinarily met with compared to the velocity of light, we learn from the quantum theory that the appropriateness of our usual causal space-time description depends entirely upon the small value of the quantum of action as compared to the actions involved in ordinary sense perceptions. Indeed, in the description of atomic phenomena, the quantum postulate presents us with the task of developing a 'complementarity' theory the consistency of which can be judged only by weighing the possibilities of definition and observation.
And again, a few paragraphs later, Bohr looks for a complementary relation between the "kinematics" of a space-time picture and the "dynamics" of a causal picture using variables like momentum, energy, etc. :
This situation would seem clearly to indicate the impossibility of a causal space-time description of the light phenomena. On one hand, in attempting to trace the laws of the time-spatial propagation of light according to the quantum postulate, we are confined to statistical considerations. On the other hand, the fulfilment of the claim of causality for the individual light processes, characterised by the quantum of action, entails a renunciation as regards the space-time description.
Once again, space-time and causality are complementary views of classical concepts.
Of course, there can be no question of a quite independent application of the ideas of space and time and of causality. The two views of the nature of light are rather to be considered as different attempts at an interpretation of experimental evidence in which the limitation of the classical concepts is expressed in complementary ways.
Bohr points out that in expressions like ΔE Δt = h and Δp Δx = h, we see both space-time (wave) variables x, t and dynamical (particle) variables E, p.

As mentioned above, Bohr thought Heisenberg's "uncertainty" could be an example of complementarity, because two different measurement apparatuses were needed to measure dynamical momentum and space-time position.

An important contribution to the problem of a consistent application of these methods has been made lately by Heisenberg (Zeitschr. f. Phys., 43, 172; 1927). In particular, he has stressed the peculiar reciprocal uncertainty which affects all measurements of atomic quantities. Before we enter upon his results it will be advantageous to show how the complementary nature of the description appearing in this uncertainty is unavoidable already in an analysis of the most elementary concepts employed in interpreting experience.

Bohr notes that Heisenberg's derivation of his indeterminacy principle was entirely done with particles and dynamical variables. Bohr then proceeds to derive Heisenberg's relations solely on the basis of a wave theory (a space-time description). This must have embarrassed Heisenberg, who resisted at first but eventually completely accepted and promoted Bohr's view of complementarity as an essential part of the Copenhagen Interpretation (along with his own uncertainty principle and Born's statistical interpretation of the wave function).

The use of a wave description reduces sharpness in definitions
Here the complementary character of the description appears, since the use of wave-groups is necessarily accompanied by a lack of sharpness in the definition of period and wave-length, and hence also in the definition of the corresponding energy and momentum as given by relation (1).

Rigorously speaking, a limited wave-field can only be obtained by the superposition of a manifold of elementary waves corresponding to all values of ν and σx, σy, σz. But the order of magnitude of the mean difference between these values for two elementary waves in the group is given in the most favourable case by the condition

Δt Δν = Δx Δσx = Δy Δσy = Δz Δσz = 1,

where Δt, Δx, Δy, Δz denote the extension of the wave-field in time and in the directions of space corresponding to the co-ordinate axes. These relations — well known from the theory of optical instruments, especially from Rayleigh's investigation of the resolving power of spectral apparatus — express the condition that the wave-trains extinguish each other by interference at the space-time boundary of the wave-field. They may be regarded also as signifying that the group as a whole has no phase in the same sense as the elementary waves. From equation (1) we find thus:

Δt ΔE = Δx ΔIx = Δy ΔIy = Δz ΔIz = h,      .      .           (2)

as determining the highest possible accuracy in the definition of the energy and momentum of the individuals associated with the wave-field. In general, the conditions for attributing an energy and a momentum value to a wave-field by means of formula (1) are much less favourable. Even if the composition of the wave-group corresponds in the beginning to the relations (2), it will in the course of time be subject to such changes that it becomes less and less suitable for representing an individual. It is this very circumstance which gives rise to the paradoxical character of the problem of the nature of light and of material particles. The limitation in the classical concepts expressed through relation (2) is, besides, closely connected with the limited validity of classical mechanics, which in the wave theory of matter corresponds to the geometrical optics, in which the propagation of waves is depicted through 'rays.' Only in this limit can energy and momentum be unambiguously defined on the basis of space-time pictures. For a general definition of these concepts we are confined to the conservation laws, the rational formulation of which has been a fundamental problem for the symbolical methods to be mentioned below.

In the language of the relativity theory, the content of the relations (2) may be summarised in the statement that according to the quantum theory a general reciprocal relation exists between the maximum sharpness of definition of the space-time and energy-momentum vectors associated with the individuals.

Bohr may still hope to "reconcile" conservation laws by claiming space-time points are "unsharp" (reminiscent of his BKS statistical conservation ideas).
This circumstance may be regarded as a simple symbolical expression for the complementary nature of the space-time description and the claims of causality. At the same time, however, the general character of this relation makes it possible to a certain extent to reconcile the conservation laws with the space-time coordination of observations, the idea of a coincidence of well-defined events in a space-time point being replaced by that of unsharply defined individuals within finite space-time regions.

To summarize, Bohr saw many elements of the new quantum mechanics as revealing his deep insight into complementarity. Among them were:

  • wave-particle duality was probably the proximate trigger, but Kant's noumena/phenomena was likely the original inspiration. And Bohr avoided referring to Einstein's years of work on wave-particle duality.
  • wave mechanics and particle/matrix mechanics as equally "true"
  • the indeterminacy principle, i.e., the reciprocal nature of the conjugate variables, momentum/position, energy/time, and action-angle
  • wave-packet limits on resolving power versus the disturbing effect of light on an observation
  • quantum systems, but apparatus described classically
  • all quantum evidence must be expressed in classical terms, "results of observations must be expressed in unambiguous language using terminology from classical physics," Heisenberg called this a paradox
  • space-time coordination and causal connection of experience (the claim of causality), space-time kinematics versus dynamical conservation laws
  • psycho-physical role of the "conscious" observer
  • "creating physical attributes by measurements" vs."disturbing phenomena by observation"
  • "renunciation of the causal space-time mode of description"
  • "individuality" irreconcilable with "causality"

In later years Bohr came to think that complementarity was important in philosophy and many other fields:

  • psycho-physical parallelism (Light and Life, 1933)
  • mind-body problem
  • biology - mechanism - vitalism
  • subject and object
  • actor and spectator
  • analysis and synthesis
  • Heisenberg's free choice of the experimenter vs. Dirac's (indeterministic) choice by Nature
  • the Eastern philosophy of yin and yang.
    The Taoist yin/yang symbol is on Bohr's gravestone
For Teachers
For Scholars

Key Components of Complementarity
  • space-time coordination and causal connection of experience (the claim of causality)
  • "renunciation of the causal space-time mode of description"
  • space-time coordination and dynamical conservation laws
  • wave-particle duality
  • the indeterminacy principle
  • reciprocal nature of conjugate variables, p,x and E,t, action-angle, h,φ
  • "individuality" irreconcilable with "causality" Dialectica/Science
  • wave-packet limits on resolving power
  • quantum systems but classical apparatus
  • "all quantum evidence must be expressed in classical terms"
  • role of the observer
  • "results of observations must be expressed in unambiguous language using terminology from classical physics'
  • psycho-physical parallelism (Light and Life, 1933
  • psychology - mind-body problem
  • biology - mechanism - vitalism
  • subject and object
  • actor and spectator
  • analysis and synthesis
  • Heisenberg free choice of experimenter vs. Dirac choice by Nature
  • "creating physical attributes by measurements" vs."disturbing phenomena by observation"

Chapter 1.1 - Creation Chapter 1.3 - Information
Home Part Two - Knowledge
Normal | Teacher | Scholar