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Topics
Introduction
Problems Freedom Knowledge Mind Life Chance Quantum Entanglement Scandals 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 Susan Blackmore 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 William Dembski Brendan Dempsey Daniel Dennett Jacques Derrida René Descartes Richard Double Fred Dretske Curt Ducasse 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 Albert Schweitzer 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 Philip W. Anderson Michael Arbib Bobby Azarian Walter Baade Bernard Baars Jeffrey Bada Leslie Ballentine Marcello Barbieri Jacob Barandes Julian Barbour Horace Barlow Gregory Bateson 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 John O. Campbell Sadi Carnot Sean B. Carroll Anthony Cashmore Eric Chaisson Gregory Chaitin Jean-Pierre Changeux Rudolf Clausius Arthur Holly Compton John Conway Simon Conway-Morris Peter Corning George Cowan 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 Theodosius Dobzhansky 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 Julian Gough Joshua Greene Dirk ter Haar Jacques Hadamard Mark Hadley Ernst Haeckel 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 Hermann von Helmholtz Grete Hermann John Herschel Francis Heylighen Basil Hiley Art Hobson Jesper Hoffmeyer John Holland 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 Bernd-Olaf Küppers Rolf Landauer Alfred Landé Pierre-Simon Laplace Karl Lashley David Layzer Joseph LeDoux Gerald Lettvin Michael Levin Gilbert Lewis Benjamin Libet David Lindley Seth Lloyd Werner Loewenstein Hendrik Lorentz Josef Loschmidt Alfred Lotka Ernst Mach Donald MacKay Henry Margenau Lynn Margulis Owen Maroney David Marr Humberto Maturana James Clerk Maxwell John Maynard Smith Ernst Mayr John McCarthy Barbara McClintock Warren McCulloch N. David Mermin George Miller Stanley Miller Ulrich Mohrhoff Jacques Monod Vernon Mountcastle Gerd B. Müller Emmy Noether Denis Noble Donald Norman Travis Norsen Howard T. Odum Alexander Oparin Abraham Pais Howard Pattee Wolfgang Pauli Massimo Pauri Wilder Penfield Roger Penrose Massimo Pigliucci Steven Pinker Colin Pittendrigh Walter Pitts Max Planck Susan Pockett Henri Poincaré Michael Polanyi Daniel Pollen Ilya Prigogine Hans Primas Giulio Prisco 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 Michael Ruse Stanley Salthe Robert Sapolsky Tilman Sauer Ferdinand de Saussure Jürgen Schmidhuber Erwin Schrödinger Aaron Schurger Sebastian Seung Thomas Sebeok Franco Selleri Claude Shannon James A. Shapiro Charles Sherrington Abner Shimony Herbert Simon Dean Keith Simonton Edmund Sinnott B. F. Skinner Lee Smolin Ray Solomonoff Herbert Spencer Roger Sperry John Stachel Kenneth Stanley Henry Stapp Ian Stewart Tom Stonier Antoine Suarez Leonard Susskind 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 Sara Imari Walker 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 CCS25 Talk Evo Devo September 12 Evo Devo October 2 Evo Devo Goodness Evo Devo Davies Nov12 |
From The Physics of Time Asymmetry to The Demon in the Machine.
Evo Devo Scholar Talk. November 12, 2025
In The Demon in the Machine: How Hidden Webs of Information Are Solving the Mystery of Life, Paul Davies doubles down on information as fundamental to understanding life.
He calls information the "missing link."
The expansion of the universe creates new possibilities of distribution faster than the atoms can work through themIn the 1977 second edition of The Physics of Time Asymmetry, Davies briefly cited Layzer's 1975 article on the Arrow of Time in Scientific American. In 1990, Layzer published his book Cosmogenesis: The Growth of Order in the Universe. The title was clearly based on Teilhard de Chardin's Cosmogenesis, which introduced his divine purpose in the nöosphere. I know that Layzer admired Teilhard. David was the adviser for my wife Holly's 1968 Ph.D. thesis Relativistic Z-Dependent Corrections to Atomic Energy Levels. Holly and I read and commented on every draft of his book. In Cosmogenesis, Layzer reiterated his model for the growth of order and drew a graph comparing the rates of universe expansion and equilibration reaction rates. He wrote, It follows that the rates of equilibrium-maintaining reactions must have exceeded the rate of cosmic expansion early in the cosmic expansion. Eventually, however, the rate of any given equilibrium-maintaining reaction must become smaller than the rate of cosmic expansion. The curve representing the reaction rate is steeper than the curve representing the expansion rate.
Based on these two simple curves and Layzer's verbal description in Scientific American and Cosmogenesis, I produced this diagram.
A few years after Cosmogenesis, Davies and two colleagues edited the 1994 volume Physical Origins of Time Asymmetry. Davies contributed the article, "Stirring up Trouble."
Without mentioning David Layzer's 1975 "Arrow of Time" article or Layzer's 1990 book on the Growth of Order, Davies coined the term "entropy gap" to describe how the maximum possible entropy goes up faster than the actual entropy (clearly this was Layzer's insight).
Does this transition from equilibrium to disequilibrium not constitute a violation of the second law of thermodynamics? No. What has happened is depicted in Fig. 3. At some time around one second, the material content of the universe was in a state of equilibrium, having the maximum possible entropy for the constraints at that time. As the universe expanded, however, the maximum possible entropy rose. The actual entropy also rose, but less fast. In particular, the relaxation time for nuclear processes to allow the cosmological material to keep pace with the changing constraints (due to the expansion) was much longer than the expansion time, so the material began to lag further and further behind equilibrium conditions ( equilibrium meaning in the nuclear case that this material is in the form of the, most stable element - iron). Hence an 'entropy gap' opened up. The continuing expansion of the universe serves to try and widen that gap slightly (though now through other processes than nucleosynthesis), while physical processes such as starlight production serves to try and narrow it.Once again Davies does not mention Layzer's work, but he develops a diagram much like mine, clearly mostly agreeing with what Layzer said. But Davies suggests (though he says he hasn't checked!) that the entropy gap will eventually close, leading to the 19th-century Kelvin-Helmholtz "heat death of the universe." David Layzer had no such pessimism. William Thomson (Lord Kelvin) was first to describe this entropy increase and it was Hermann Helmholtz called it the “heat death” of the universe. But did the universe begin with "low entropy" and lots of information as they thought?
Here we should review a short clip from the excellent Veritasium presentation mentioned on Edu-Talk a few weeks ago. (We need to skip over the ads!)
"ENTROPY: The Most Misunderstood Concept in Physics" The Veritasium clip includes the Past Hypothesis, which Kelvin, Helmholtz, James Clerk Maxwell, Ludwig Boltzmann and many others since, believed meant that the universe began with a high degree of organization or order (negative entropy or information) and that it has been running down ever since as positive entropy increases. As we see clearly, both Layzer and Davies agree that the entropy at the universe origin was much lower than the entropy today. They also clearly label that early entropy as maximum entropy for the extreme density and temperature conditions at the origin. So there was no room for any information at the beginning of the universe.. In chapter 6 of Demon in the Machine, Davies writes... The universe abounds in complexity, from everyday systems such as turbulent streams and snowflakes to grand cosmic structures like nebulae and spiral galaxies. However, one class of complex systems – life – stands out as especially remarkable. In his Dublin lectures Schrödinger identified life’s ability to buck the trend of the second law of thermodynamics as a defining quality. Living organisms achieve this entropy-defying feat by garnering and processing information and directing it into purposeful activity. By coupling patterns of information to patterns of chemical reactions, using demons to achieve a very high degree of thermodynamic efficiency, life conjures coherence and organization from molecular chaos. One of the greatest outstanding questions of science is how this unique arrangement came about in the first place.We must clarify "life's ability to buck the trend of the second law." It is not an "entropy-defying feat." done "by garnering and processing information and directing it into purposeful activity." All that Schrödinger's "What Is Life" said in 1944 was that life “feeds on negative entropy.” It is this source of negative entropy, or free energy, i.e., energy available to do work, that allows living things to communicate with their body parts and with other living things, to process information (though without computer processing), and to act purposefully. 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. I made a crude still illustration of solar photons coming to Earth.
This conversion of high energy photons to low energy is again illustrated much more beautifully by Veritasium's
"ENTROPY"
But Schrödinger didn't know how the Sun (and all the stars) came to be such a source of negative entropy or free energy.
Following Eddington and Layzer (and now Davies), I've explained how a star can become a source of free energy with what I'm calling the cosmic creation process.
The expansion of space created new possible locations in phase-space, producing pockets of negative entropy. When an actual information structure forms locally, it will not be stable unless it radiates away positive entropy to satisfy the second law globally.
Two steps, first possibilities, then one actuality, are the core of the cosmic creation process.
These two steps or two stages are first indeterministic (random) possibilities, second an adequately determined (not pre-determined!) choice or selection.
This is exactly how Claude Shannon's theory of the communication of information works, showing the intimate connection between negative entropy and information!
Information philosophy identifies four such processes creating new information. They are all driven by random possibilities followed by one selected as actual.
From the Origin of the Universe to Life on Other Planets
The universe began with primeval quarks, gluons, electrons, and photons. In the first few minutes after the origin, the cosmic creation process produced the earliest information structures, protons and neutrons. 380,000 years later, the ionized plasma cooled to the surface temperature of the Sun and allowed those protons and electrons to form atoms, making the universe transparent. That allows us today to see back in time to the cosmic microwave background., now cooled to 2.7K.
Galaxies, stars, and planets began to form about 400 million years after the origin.
The Sun, a population I star, formed only about 4.5 billion years ago, along with its planets, and life emerged rather quickly about a half-billion years later.
The Sun will continue to support life on Earth for another 5 billion years, after which it will grow into a red giant star whose surface will reach to Earth's orbit.
Well before then, humans will have populated Mars. And, in the unlikely case that we have not yet connected with any extraterrestrial intelligent life, we will have seeded life on many exoplanets within habitable zones and long-lived stars like brown dwarfs.
Giulio Prisco, who did research with the European Space Agency, and I, who advised NASA on its Long Range Program in Space Astronomy, have some suggestions for future space exploration
In his book Futurist Spaceflight Meditations, Prisco writes...
We must strenuously push toward our cosmic destiny among the stars. Beginning to expand beyond the Earth before it’s too late is our most important task at this moment in history. Many actors have important roles to play, and there’s room for everyone...Our suggestions...
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