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Philosophers

Mortimer Adler
Rogers Albritton
Alexander of Aphrodisias
Samuel Alexander
William Alston
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Anselm
Louise Antony
Thomas Aquinas
Aristotle
David Armstrong
Harald Atmanspacher
Robert Audi
Augustine
J.L.Austin
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Alexander Bain
Mark Balaguer
Jeffrey Barrett
William Barrett
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Henri Bergson
George Berkeley
Isaiah Berlin
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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
Lawrence Cahoone
C.A.Campbell
Joseph Keim Campbell
Rudolf Carnap
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Nancy Cartwright
Gregg Caruso
Ernst Cassirer
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Cicero
Tom Clark
Randolph Clarke
Samuel Clarke
Anthony Collins
Antonella Corradini
Diodorus Cronus
Jonathan Dancy
Donald Davidson
Mario De Caro
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Jacques Derrida
René Descartes
Richard Double
Fred Dretske
John Dupré
John Earman
Laura Waddell Ekstrom
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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
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R.E.Hobart
Thomas Hobbes
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Shadsworth Hodgson
Baron d'Holbach
Ted Honderich
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Ferenc Huoranszki
Frank Jackson
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Tomis Kapitan
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Jaegwon Kim
William King
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Christine Korsgaard
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Joseph Levine
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David Lewis
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C. Lloyd Morgan
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Arthur O. Lovejoy
E. Jonathan Lowe
John R. Lucas
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Ruth Barcan Marcus
Tim Maudlin
James Martineau
Nicholas Maxwell
Storrs McCall
Hugh McCann
Colin McGinn
Michael McKenna
Brian McLaughlin
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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.Nowell-Smith
Robert Nozick
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Timothy O'Connor
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Charles Sanders Peirce
Derk Pereboom
Steven Pinker
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Paul Russell
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David Shiang
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Henry Sidgwick
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J.J.C.Smart
Saul Smilansky
Michael Smith
Baruch Spinoza
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Isabelle Stengers
George F. Stout
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Peter Strawson
Eleonore Stump
Francisco Suárez
Richard Taylor
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Kadri Vihvelin
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R. Jay Wallace
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Roy Weatherford
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Alfred North Whitehead
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David Wiggins
Bernard Williams
Timothy Williamson
Ludwig Wittgenstein
Susan Wolf

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David Albert
Michael Arbib
Walter Baade
Bernard Baars
Jeffrey Bada
Leslie Ballentine
Marcello Barbieri
Gregory Bateson
Horace Barlow
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
Jean-Pierre 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
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Louis de Broglie
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Hans Driesch
John Eccles
Arthur Stanley Eddington
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Manfred Eigen
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Hugh Everett, III
Franz Exner
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R. A. Fisher
David Foster
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Philipp Frank
Steven Frautschi
Edward Fredkin
Augustin-Jean Fresnel
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
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Dirk ter Haar
Jacques Hadamard
Mark Hadley
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Sam Harris
Ralph Hartley
Hyman Hartman
Jeff Hawkins
John-Dylan Haynes
Donald Hebb
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Basil Hiley
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Pascual Jordan
Eric Kandel
Ruth E. Kastner
Stuart Kauffman
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William R. Klemm
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Leopold Kronecker
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Franco Selleri
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Dean Keith Simonton
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Francisco Varela
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Heinz von Foerster
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John B. Watson
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Paul A. Weiss
Herman Weyl
John Wheeler
Jeffrey Wicken
Wilhelm Wien
Norbert Wiener
Eugene Wigner
E. O. Wilson
Günther Witzany
Stephen Wolfram
H. Dieter Zeh
Semir Zeki
Ernst Zermelo
Wojciech Zurek
Konrad Zuse
Fritz Zwicky

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Dirk ter Haar
Dirk ter Haar was a Dutch physicist who studied physics in Scotland (St. Andrews) and England (Oxford).,

During the last years of World War II he attended Hendrik Kramers' famous lectures on statistical mechanics, which led to the great school of Dutch statistical physicists (F. J. Belinfante, Max Dresden, Nico van Kampen, Abraham Pais).

After the war he went to study at Niels Bohr's Institute in Copenhagen, then went back to Leiden to receive the Ph.D. under Hendrik Kramers,

His academic career was spent largely at the University of Oxford. One of his students was the historian of statistical physics Steven Brush.

He wrote a number of important books on statistical mechanics in the 1950's and one on the Old Quantum Theory in 1967. Perhaps his most famous book was the 1954 Elements of Statistical Mechanics, which ter Haar said was largely a new version of of the Kramers lectures in 1944-45.

ter Haar considered the implications of quantum mechanics for statistical mechanics. Many statistical physicists argued that quantum mechanics requires no changes to the conclusions of classical thermodynamics and statistical mechanics. These thinkers tended to be determinists who were uncomfortable with Werner Heisenberg's claim that quantum mechanics had eliminated causality in physics.

ter Haar also challenged the applicability of Claude Shannon's information theory and Norbert Wiener's cybernetics to statistical mechanics. But he accepted Leo Szilard's analysis of Maxwell's demon for a single particle, showing how a measurement of a single particle involves k ln2 of entropy, or one bit of information, and Leon Brillouin's analysis, where he coined the term "negentropy."

He wrote...

The relationship was introduced because Boltzmann's formula for entropy is identical to Shannon's formula with a minus sign.
S = k ∑ pi ln pi.
If all pi are identical,S = k ln W.
Information is neither matter nor energy, but where an information structure is present, entropy is low and Gibbs free energy is high.
The relationship between entropy and lack of information has led many authors, notably Shannon, to introduce “entropy” as a measure for the information transmitted by cables and so on, and in this way entropy has figured largely in recent discussions in information theory.

It must be stressed here that the entropy introduced in information theory is not a thermodynamical quantity and that the use of the same term is rather misleading. It was probably introduced because of a rather loose use of the term “information.”

In this connection we may briefly discuss Maxwell’s demon. Maxwell introduced in 1871 his famous demon, “a being whose faculties are so sharpened that he can follow every molecule in its course, and would be able to do what is at present impossible to us. . . . Let us suppose that a vessel is divided into two portions A and B by a division in which there is a small hole, and that a being who can see the individual molecules opens and closes this hole, so as to allow only the swifter molecules to pass from A to B, and only the slower ones to pass from B to A. He will, thus, without expenditure of work raise the temperature of B and lower that of A, in contradiction to the second law of thermodynamics.”

Maxwell’s demon has been widely discussed and various authors have set out to show that various attempts to circumvent the second law by using the demon are bound to fail. Although their discussions differ in some respects they have a few points in common. The first point is the observation that one should take the demon to be part of the total system and then one must consider the total entropy of the original system and the demon. The second point which was most clearly developed for the first time by Szilard is that the demon, in order to be able to operate the trapdoor through which the molecules pass, must receive information. Its own entropy increases therefore and it is now the question whether the increase of the demon’s entropy is smaller or larger than the decrease of the entropy of the gas. Both Szilard and Brillouin consider possible arrangements and show that in those cases the net change of entropy is positive. Szilard analyzes the problem very thoroughly and shows that one can describe a generalized Maxwell’s demon as follows. By some means an operation on a system is determined by the result of a measurement on the system which immediately precedes the operation. In Maxwell’s original scheme the operation was the opening of the trapdoor and the measurement was the determination of the velocity of an approaching molecule. The result of the operation will be a decrease of entropy, but the preceding measurement will be accompanied by an increase in entropy, and once again one must consider the balance. Wiener takes a simpler point of view.; He considers the situation, where the demon acts, as a metastable state and writes: “In the long run, the Maxwell demon is itself subject to a random motion corresponding to the temperature of its environment and it receives a large number of small impressions until it falls into ‘a certain vertigo’ and is incapable of clear perceptions. In fact, it ceases to act as a Maxwell demon.”

This point of view is probably too simplified and we prefer that of Szilard’s and refer the reader to his paper for a more extensive discussion.

We can note that in the most widely used modern textbook on statistical physics, Fred Reif says,

The quantity —In Γ, i.e., the function Σ Pr In Pr, can be used as a measure of nonrandomness, or information, available about systems in the ensemble.

This function plays a key role as a measure of information in problems of communication and general “information theory.”*

* See, for example, L. Brillouin, “Science and Information Theory,” 2d ed., Academic Press, New York, 1962; or J. R. Pierce, “Symbols, Signals, and Noise,” Harper, New York, 1961. Statistical mechanics is considered from the point of view of information theory by E. T. Jaynes in Phys. Rev., vol. 106, p. 620 (1957).
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