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 Bois-Reymond Hilary Bok Laurence BonJour George Boole Émile Boutroux Daniel Boyd F.H.Bradley C.D.Broad Michael Burke Jeremy Butterfield Lawrence Cahoone C.A.Campbell Joseph Keim Campbell Rudolf Carnap Carneades Nancy Cartwright Gregg Caruso Ernst Cassirer David Chalmers Roderick Chisholm Chrysippus Cicero Tom Clark Randolph Clarke Samuel Clarke Anthony Collins August Compte Antonella Corradini Diodorus Cronus Jonathan Dancy Donald Davidson Mario De Caro Democritus Daniel Dennett Jacques Derrida René Descartes Richard Double Fred Dretske 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 Niels Henrik Gregersen 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 James Ladyman 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 Ernest Nagel Thomas Nagel Otto Neurath 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 U.T.Place 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 John Duns Scotus Arthur Schopenhauer John Searle Wilfrid Sellars David Shiang Alan Sidelle Ted Sider Henry Sidgwick Walter Sinnott-Armstrong Peter Slezak 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 Xenophon Scientists David Albert Michael Arbib Walter Baade Bernard Baars Jeffrey Bada Leslie Ballentine Marcello Barbieri Jacob Barandes Gregory Bateson Horace Barlow John S. Bell Mara Beller Charles Bennett Ludwig von Bertalanffy Susan Blackmore Margaret Boden David Bohm Niels Bohr Ludwig Boltzmann John Tyler Bonner Emile Borel Max Born Satyendra Nath Bose Walther Bothe Jean Bricmont Hans Briegel Leon Brillouin Daniel Brooks Stephen Brush Henry Thomas Buckle S. H. Burbury Melvin Calvin William Calvin Donald Campbell Sadi Carnot Anthony Cashmore Eric Chaisson Gregory Chaitin Jean-Pierre Changeux Rudolf Clausius Arthur Holly Compton John Conway Simon Conway-Morris Peter Corning Jerry Coyne John Cramer Francis Crick E. P. Culverwell Antonio Damasio Olivier Darrigol Charles Darwin Paul Davies Richard Dawkins Terrence Deacon Lüder Deecke Richard Dedekind Louis de Broglie Stanislas Dehaene Max Delbrück Abraham de Moivre David Depew Bernard d'Espagnat Paul Dirac Hans Driesch John Dupré John Eccles Arthur Stanley Eddington Gerald Edelman Paul Ehrenfest Manfred Eigen Albert Einstein George F. R. Ellis Walter Elsasser Hugh Everett, III Franz Exner Richard Feynman R. A. Fisher David Foster Joseph Fourier George Fox Philipp Frank Steven Frautschi Edward Fredkin Augustin-Jean Fresnel Karl Friston Benjamin Gal-Or Howard Gardner Lila Gatlin Michael Gazzaniga Nicholas Georgescu-Roegen 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 John-Dylan Haynes Donald Hebb Martin Heisenberg Werner Heisenberg Grete Hermann John Herschel Basil Hiley Art Hobson Jesper Hoffmeyer Don Howard John H. Jackson Ray Jackendoff Roman Jakobson E. T. Jaynes William Stanley Jevons 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 Pierre-Simon Laplace Karl Lashley David Layzer Joseph LeDoux Gerald Lettvin Gilbert Lewis Benjamin Libet David Lindley Seth Lloyd Werner Loewenstein Hendrik Lorentz Josef Loschmidt Alfred Lotka Ernst Mach Donald MacKay Henry Margenau Owen Maroney David Marr Humberto Maturana James Clerk Maxwell John Maynard Smith Ernst Mayr John McCarthy Warren McCulloch N. David Mermin George Miller Stanley Miller Ulrich Mohrhoff Jacques Monod Vernon Mountcastle Emmy Noether Donald Norman Travis Norsen Howard T. Odum Alexander Oparin Abraham Pais Howard Pattee Wolfgang Pauli Massimo Pauri Wilder Penfield Roger Penrose Steven Pinker Colin Pittendrigh Walter Pitts Max Planck Susan Pockett Henri Poincaré Daniel Pollen Ilya Prigogine Hans Primas Zenon Pylyshyn Henry Quastler Adolphe Quételet Pasco Rakic Nicolas Rashevsky Lord Rayleigh Frederick Reif Jürgen Renn Giacomo Rizzolati A.A. Roback Emil Roduner Juan Roederer Robert Rosen Frank Rosenblatt Jerome Rothstein David Ruelle David Rumelhart Stanley Salthe Robert Sapolsky Tilman Sauer Ferdinand de Saussure Jürgen Schmidhuber Erwin Schrödinger Aaron Schurger Sebastian Seung Thomas Sebeok Franco Selleri Claude Shannon Charles Sherrington Abner Shimony Herbert Simon Dean Keith Simonton Edmund Sinnott B. F. Skinner Lee Smolin Ray Solomonoff Roger Sperry John Stachel Kenneth Stanley Henry Stapp Tom Stonier Antoine Suarez Leo Szilard Max Tegmark Teilhard de Chardin Libb Thims William Thomson (Kelvin) Richard Tolman Giulio Tononi Peter Tse Alan Turing Robert Ulanowicz C. S. Unnikrishnan Nico van Kampen Francisco Varela Vlatko Vedral Vladimir Vernadsky Clément Vidal Mikhail Volkenstein Heinz von Foerster Richard von Mises John von Neumann Jakob von Uexküll C. H. Waddington James D. Watson John B. Watson Daniel Wegner Steven Weinberg August Weismann Paul A. Weiss Herman Weyl John Wheeler Jeffrey Wicken Wilhelm Wien Norbert Wiener Eugene Wigner E. O. Wiley E. O. Wilson Günther Witzany Carl Woese Stephen Wolfram H. Dieter Zeh Semir Zeki Ernst Zermelo Wojciech Zurek Konrad Zuse Fritz Zwicky Presentations Biosemiotics Free Will Mental Causation James Symposium Evo Devo Scholar Talk CSC25 Talk |
The Astrophysics and the Cosmology
We have twenty minutes to explain how a complex system can increase its complexity, get more complicated, get more organized, and increase its information content.
First, I need to ask you all a couple of questions. I assume you all know the second law of thermodynamics. Entropy always increases!. Disorder increases. Everyone OK with that? It's called the Arrow of Time. Information is always being lost, right?
OK, We have an enormous amount of information in the world today. Ten major companies in the US are investing billions of dollars to put all our knowledge in their new AI data centers! (Half of all US business investment os going into AI.) And this info is not counting all the biological information, the planetary information, and the information in all the stars and 1011 galaxies!
Second question!
How much information do you think there was at the origin of the universe?
Many people think there was a lot! Because it's been running down ever since the beginning of time and we still have a lot. Ludwig Boltzmann thought this.
How many of you think the universe had the exact same amount of information at the beginning as we have today? The idea is that just like energy is conserved and total matter is a perfectly conserved quantity, this idea is that information itself is a conserved constant. How many like that idea? Same information at all times!
Many organized religions think this is the case. Almighty God is omnipotent and omniscient. In-sha-allah!
My MIT colleague Seth Lloyd thinks this is the case.
He also thinks the universe is a computer! How many of you think the universe might be a computer?
How many of you think man is a machine and the mind is a computer? This is actually the most popular theory among cognitive neuroscientists today! And many AI experts too. How many of you think your mind is a computer?
But back to the information at the universe origin. How many of you know Laplace's Demon?
Laplace's demon implies that the past, the present, and the future always contain exactly the same knowledge. This makes information a constant of nature.
of Self-Organization in Complex Systems ![]() ![]() ![]() Complexity Science studies all of them. It also studies Life, but there’s a vital difference between living things and the abiotic universe. The difference is the role of information. The universe and its galaxies, stars, and planets are all rich in abstract immaterial information. But this immaterial information needs matter to be embodied and energy to be communicated for scientists to observe and measure that information! All the objects in the universe are concrete material information structures, composed of matter and energy components, from the quarks, gluons, electrons, and photons present at the origin, through the atoms, molecules, and macromolecules that could not be stable until the universe cooled to the current surface temperature of the Sun (about 6000K), 380 thousand years after the origin of the universe. Non-living objects like atoms, molecules, planets, stars, and galaxies are passive information structures. They are entirely controlled by fundamental physical forces - the strong and weak nuclear forces, electromagnetism, and gravitation. These objects do not control themselves. They are reducible to physical causes. They are not acting. They are acted upon. Living things, you and I, are active dynamic growing information structures, forms through which matter and energy continuously flow. And the top-down communication of biological information controls those flows! The communication of information between living things gives rise to social structures, from slime-molds to political parties. Single-cell, plant, and animal awareness of (i.e., communication with) information in their environment culminates in human consciousness. The storage of information in the minds of humans and their artifacts (from books to the Internet) is the sum of all knowledge. Now the fundamental laws of thermodynamics apply to both living and non-living systems. The second law says that entropy (disorder) must always increase, suggesting a "heat death" for the universe. It also suggests the universe must have begun with a vast amount of information. We will show how the universe began with a bare minimum of information. And we'll explain how it avoids a "heat death" To increase the complexity of any system, including the universe, it must generate or incorporate new information - "negative entropy." Erwin Schrödinger famously argued in his 1944 article "What Is Life?" that life “feeds on negative entropy.” I like to call this Schrödinger's Rule: No Growth Without A Negentropy Source. Schrödinger’s source for negative entropy was our Sun. With the bright Sun as a heat source and the dark night sky as a heat sink, the Earth is a thermodynamic engine. ![]() ![]()
Information in Biology
In his 1944 "What Is Life" article, Schrödinger also explained how genetic information could be stored in the atomic structure of a long molecule or "periodic crystal." That molecule was found to be DNA just nine years later by James Watson and Francis Crick in 1953.
Just three years before information in the genetic code was discovered, Claude Shannon formulated his theory of thecommunication of information, describing digital "bits" of information as 1's and 0's (or yes and no answers to questions). Shannon said that the amount of information communicated depends on the number of possible messages. With eight possible messages, one actual message communicates three bits of information (2³ = 8).
If there is only one possible message, there is no new information. This corresponds to the deterministic view that there is only one possible future!. Both that future and the entire past are completely pre-determined from the beginning of time, and the total information in the universe is a conserved constant, as many physicists, and some world religions, believe.
I call this Shannon's Principle: No New Information Creation Without Possibilities.
Again inspired by Arthur Stanley Eddington, who suggested in 1928 that Werner Heisenberg’s uncertainty principle could put a “chink” in determinism, Layzer and I debated about free will.
In the 1970’s I came up with a “two-stage model” of free will, the first stage alternative possibilities, the second stage adequately determined decisions or choices. Researching the literature for years since then. I’ve now identified many philosophers and scientists who proposed the same two-stage model, well before me and after me.
See informationphilosopher.com/freedom/two-stage_models.html
I’ve since extended this two-stage model of first possibilities, then actualities to all the processes in the universe that create all new information and information structures.
I call it the cosmic creation process. It starts with Eddington and Layzer’s insight into the growth of order in the universe.
See informationphilosopher.com/introduction/creation.
The cosmic creation process also describes Darwinian evolution. Consider the evolutionary biologist Ernst Mayr, in his 1988 book Toward a New Philosophy of Biology.
Evolutionary change in every generation is a two-step process: the production of genetically unique new individuals and the selection of the progenitors of the next generation. The important role of chance at the first step, the production of variability, is universally acknowledged, but the second step, natural selection, is on the whole viewed rather deterministically: Selection is a non-chance process.We now have three processes that need two stages or steps to create something new -
Abstract
I introduce my cosmic creation process, which consists of two stages or steps, first the ontologically random generation of alternative possibilities, followed by the adequately determined selection of one actual outcome.
I describe how the cosmic creation process does not violate the second law of thermodynamics. I'll show how the universe avoids a "heat death," without violating the second law of thermodynamics. I’ll also compare the cosmic creation process to complexity science, to complex systems, and to complex adaptive systems.
I show how this two-stage creative process helps to explain three great problems in philosophy and science. If there is time, I’ll add a fourth (Einstein) and mention two more new ideas.
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