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 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
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
Sadi Carnot
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
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
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
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
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
Barabara McClintock
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
Ian Stewart
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
CCS25 Talk
 
Evo Devo Universe Scholar Talk, September 12, 2025

My Background
When I came to Harvard in 1958, I had studied physics at Brown, reading about entropy in Arthur Stanley Eddington's The Nature of the Physical World, his 1927 Gifford Lectures.

The entropy law, the second law of thermodynamics, isn't like all the other physical laws, Eddington said. For one thing, it isn't time reversible like Newton's laws. For another, it has qualities unlike any other physical quantity, it feels more like beauty or harmony.
Maybe it's something like good and evil, I thought.

I asked all my professors a question, "if the universe began in a state of thermal equilibrium, maximum entropy, how can we have so much information in the world today?"

Only two professors took me seriously. One was David Layzer. He spent the rest of his life on the problem. I've been reading philosophy and physics for seventy years to explain it.

Does the Universe Develop and Evolve?

Of course it does. We study Cosmic Evolution (Eric Chaisson’s book), including
Galactic Evolution, Stellar Evolution, and Planetary Evolution.

Now Planets, Stars, Galaxies, and the Universe itself are all Complex Systems.
Complexity Science studies all of them.

Since Georgi's satellite meeting on complexity science last week in Siena, where I had hoped to meet Paul Davies, I've drafted a brief history of complex systems showing how Davies turned the Santa Fe Institute toward theology and teleology.

Of course Life is also a complex system, but I want to discuss 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. This immaterial information needs matter to be embodied and energy
to be communicated, for scientists to observe and to 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 (around 6000K),
about 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.

But living things, you and I, are active dynamic growing information structures, we are forms through which matter and energy continuously flow. And it's the top-down communication
of biological information that controls those flows!

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 began with a vast amount of information, since increasing entropy has been decreasing information since the origin and there's so much left today.

But I'll show how the universe began with a bare minimum of information.
And I'll explain how it avoids that "heat death."

First we need to consider Laplace's Demon.

Pierre Simon Laplace knew Newton's Laws of classical mechanics extremely well.

He imagined an intelligent demon who knows the positions and the velocities of every particle in the universe and the demon knows the forces on all those particles.
The demon could then know the entire past and the future of the universe.

In that case, information would be a constant of nature (plotted as the blue line below).
My MIT colleague Seth Lloyd thinks information is a conserved constant, like the conservation laws for mass and energy. He also thinks the universe is a computer!

However, midway through the 19th century, Lord Kelvin realized that the then just discovered second law of thermodynamics requires that information can not be constant. It would be being destroyed as the entropy irreversibly increases.

The physicist Hermann Helmholtz described this as the "heat death" of the universe.

Now Kelvin’s claim of a "heat death" would be correct if the universe were a closed system.
But it's not closed. The universe is open and infinite. We'll see how an open universe can actually create negative entropy locally to avoid thermal equilibrium.

In his famous 1944 article "What Is Life?," Erwin Schrödinger famously argued that life “feeds on negative entropy.”

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.

But Schrödinger didn't know how the Sun came to be such a source of negative entropy.

That’s a problem for cosmology. We need to explain how a universe beginning in thermal equilibrium with maximum entropy (total disorder) can create a spherically symmetric star sending a stream of negative entropy to Earth.

Arthur Stanley Eddington was the great scientist who proved Albert Einstein's general relativity claim that space is curved at a 1919 eclipse expedition (making Einstein famous).

Eddington suggested in 1934 that the universe expansion, discovered by Edwin Hubble in 1927, might create new "phase-space" cells faster than the particles can randomly fill those cells and maximize the entropy.

Note that the universe could allow local reductions in the entropy, what I called "pockets" of negative entropy, but only if the global entropy elsewhere is increased even more to satisfy the second law of thermodynamics.

In his 1989 book Cosmogenesis, my Harvard mentor David Layzer developed Eddington's idea. Layzer showed that the maximum possible entropy of the expanding universe increases much faster than the actual entropy increases. Disorder (entropy) and order (negative entropy) are simultaneously increasing in the universe.

I adapted the diagrams in Layzer’s book to create this picture of his Growth of Information.

Between the actual entropy and the maximum possible entropy you can see there's plenty of room for galaxies, stars, and planets to form.

Notice that the universe didn't have a lot of information at the origin. It also didn't have the same information that it has today, as Laplace and my MIT colleague Seth Lloyd believe. Lloyd also believes the universe is a computer!

The expansion of the universe creates new space, which means there are many more possible "phase-space" cells where particles can actually be distributed.

I decided to call this the Cosmic Creation Process, based on Eddington and Layzer’s insight into the growth of order in the universe.

My Cosmic Creation Process is the first of four examples of random possibilities being created that can lead to new information in the universe.

The others are

I call these all "two-stage models." First possibilities, then a new actuality.

In the first stage new possibilities randomly appear.

In the second stage one possibility becomes actual.

Biological Information and Its Communication

In his famous 1944 article "What Is Life", Erwin Schrödinger also explained how genetic information could be stored in the atomic structure of a long molecule or "aperiodic 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 the communication 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.

The Problem of Free Will
Again inspired by Arthur Stanley Eddington, who suggested in 1928 that Werner Heisenberg’s uncertainty principle could put a “chink” in determinism, David Layzer and I debated about the free will problem.

In the 1970’s I came up with my “two-stage model” of free will, in the first stage alternative possibilities randomly come to mind, in the second stage the agent makes 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.

Over the years I debated the problem of free will with the libertarian philosopher Robert Kane and the determinist/compatibilist philosopher Daniel Dennett. Time permitting in the discussion, I'll tell you more about them.

A Two-Stage Model for Evolution

In the 1990's I extended my two-stage model of first possibilities, then actualities to all the processes in the universe that create all new information and information structures. This obviously included Darwinian evolution. Here is the evolutionary biologist Ernst Mayr describing the two-step process.

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.

Now all complex adaptive systems are obviously creative. And the self-organizing autopoetic description of Umberto Maturana and Francesco Varela obviously describes them perfectly. But the “self” in a Benard cell is not communicating information to its component atoms.
It has no thoughts, no intention, no goals, no purpose.

A Benard cell is a passive information structure, reducible to its components. True, it is a dissipative structure, at the edge of chaos, as Ilya Prigogine saw, but it is not alive. And finally also true, the autocatalytic process is top-down causation controlling or constraining lower level processes. These top-down forces are purely physical. Benard cells are not alive.

As I see it, Purpose and Values and Meanings all enter the universe when Life appears.

The only place in the universe where life is known to exist is our biosphere, first named by the Austrian chemist Edward Seuss in the nineteenth century as the interface of the lithosphere and lower atmosphere.

In the twentieth century, the biosphere was made more popular by Vladimir Vernadsky, who inspired Teilhard de Chardin's noösphere. And today the biosphere is the locus of James Lovelock and Lynn Margulis' Gaia Hypothesis.

If there exists an entity which has provided us with everything, to which we should be thankful, even reverential, it is surely the biosphere, which is our home in the universe.

Summary
I introduced 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 described how the cosmic creation process does not violate the second law of thermodynamics. And I showed how the universe avoids a "heat death," without violating the second law of thermodynamics.

I claimed this two-stage creative process helps to explain three great problems in philosophy and science.

  1. The problem of free will and determinism.
  2. Shannon’s communication of information.
  3. Darwin’s theory of natural selection

I've made four more original contributions to science that might be of interest.

  1. A biological model of the mind as an Experience Recorder and Reproducer and the problem of learned representation in AI.
  2. The “weird” problem of Quantum Entanglement, which creates two “bits” of information instantly at widely separated locations, without "spooky action at a distance."
  3. The Flatness of the Universe, that average spatial curvature may be zero, as confirmed by Steven Weinberg in his text Cosmology.
  4. The Origin of Irreversibility, based on Einstein's 1916 paper on the absorption and emission of radiation, which was the basis of my Ph.D. thesis.

All my work is available on my website informationphilosopher.com

My personal story is here - informationphilosopher.com/about

The ERR model is here informationphilosopher.com/mind/err/

Entanglement is discussed here - informationphilosopher.com/entanglement/common_cause/

You can contact me here bobdoyle@informationphilosopher.com

Normal | Teacher | Scholar