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
Lawrence Cahoone
C.A.Campbell
Joseph Keim Campbell
Rudolf Carnap
Carneades
Nancy Cartwright
Gregg Caruso
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
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
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
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
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
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
C.F. von Weizsäcker
William Whewell
Alfred North Whitehead
David Widerker
David Wiggins
Bernard Williams
Timothy Williamson
Ludwig Wittgenstein
Susan Wolf

Scientists

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
Lüder Deecke
Richard Dedekind
Louis de Broglie
Stanislas Dehaene
Max Delbrück
Abraham de Moivre
Bernard d'Espagnat
Paul Dirac
Hans Driesch
John Eccles
Arthur Stanley Eddington
Gerald Edelman
Paul Ehrenfest
Manfred Eigen
Albert Einstein
George F. R. Ellis
Hugh Everett, III
Franz Exner
Richard Feynman
R. A. Fisher
David Foster
Joseph Fourier
Philipp Frank
Steven Frautschi
Edward Fredkin
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
John Herschel
Basil Hiley
Art Hobson
Jesper Hoffmeyer
Don Howard
John H. Jackson
William Stanley Jevons
Roman Jakobson
E. T. Jaynes
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
Hendrik Lorentz
Werner Loewenstein
Josef Loschmidt
Ernst Mach
Donald MacKay
Henry Margenau
Owen Maroney
David Marr
Humberto Maturana
James Clerk Maxwell
Ernst Mayr
John McCarthy
Warren McCulloch
N. David Mermin
George Miller
Stanley Miller
Ulrich Mohrhoff
Jacques Monod
Vernon Mountcastle
Emmy Noether
Donald Norman
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
Emil Roduner
Juan Roederer
Jerome Rothstein
David Ruelle
David Rumelhart
Tilman Sauer
Ferdinand de Saussure
Jürgen Schmidhuber
Erwin Schrödinger
Aaron Schurger
Sebastian Seung
Thomas Sebeok
Franco Selleri
Claude Shannon
Charles Sherrington
David Shiang
Abner Shimony
Herbert Simon
Dean Keith Simonton
Edmund Sinnott
B. F. Skinner
Lee Smolin
Ray Solomonoff
Roger Sperry
John Stachel
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
Francisco Varela
Vlatko Vedral
Mikhail Volkenstein
Heinz von Foerster
Richard von Mises
John von Neumann
Jakob von Uexküll
C. S. Unnikrishnan
C. H. Waddington
John B. Watson
Daniel Wegner
Steven Weinberg
Paul A. Weiss
Herman Weyl
John Wheeler
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

Presentations

Biosemiotics
Free Will
Mental Causation
James Symposium
 
Stephen Brush

Stephen G. Brush is a historian of science who has documented the history of the kinetic theory of gases. He translated from German some of Ludwig Boltzmann's major works on the second law of thermodynamics.

In an important 1976 contribution to the Journal of the History of Ideas, Brush argues that many nineteenth-century scientists accepted chance and randomness at the atomic level and that they related it to irreversibility in natural phenomena. (Other historians, e.g., Ian Hacking, made similar claims at the same time.)

In reading the casual remarks, and even what seem to be carefully considered pronouncements by nineteenth-century scientists, the twentieth-century reader often finds a puzzling ambiguity. Words like randomness, irregularity, and indeterminism may appear to imply that molecules or other entities do not move in paths that are completely determined by the positions, velocities, and forces of all particles in the system; yet the same author may express himself in a manner that is completely consistent with the view that these paths really are determined but we simply cannot obtain complete knowledge of them. What we might now call a crucial distinction between ontological and epistemological indeterminism is frequently blurred in these writings. This ambiguity can be used to argue that almost every one of the scientists quoted here believed only in epistemological, not ontological randomness—but such an argument would conceal a gradual but extremely significant historical shift in the meaning of concepts.
(Irreversibility and Indeterminism: Fourier to Heisenberg, Journal of the History of Ideas, 1976, reprinted in Kinetic Theory of Gases, Imperial College Press, 2003, p.604)

Brush thus sees more continuity in the idea of indeterminism than typical historians of modern quantum physics who situate the beginnings of indeterminism in quantum mechanics and Werner Heisenberg's indeterminacy principle. Although he notes that many nineteenth-century scientists thought that chance was not ontologically real but rather merely epistemic, a consequence of the limits on human knowledge.

It is generally recognized that statistical ideas and methods were first introduced into physics in connection with the kinetic theory of gases. At the same time, modern writers invariably point out that in this case statistics was used only as a matter of convenience in dealing with large numbers of particles whose precise positions and velocities at any instant are unknown, or, even if known, could not be used in practice to calculate the gross behavior of the gas. Nevertheless, it is claimed, nineteenth-century physicists always assumed that the gas is really a deterministic mechanical system, so that if the super-intelligence imagined by Laplace were supplied with complete information about all the individual atoms at one time he could compute their positions and motions at any other time as well as the macroscopic properties of the gas. As Laplace himself had written in 1783, "The word 'chance,' then expresses only our ignorance of the causes of the phenomena that we observe to occur and to succeed one another in no apparent order." This situation is to be sharply distinguished, according to the usual accounts of the history of modern physics, from the postulate of atomic randomness or indeterminism which was adopted only in the 1920's in connection with the development of quantum mechanics. Thus, part of the "scientific revolution" that occurred in the early twentieth century is supposed to have been a discontinuous change from classical determinism to quantum indeterminism.

While I think it is legitimate to say that a revolution in physical thought has occurred since about 1800, I do not believe it is accurate to localize it in the two or three decades at the beginning of the twentieth century. Some of the most dramatic events did take place during that period, but they could not have had the impact they actually did if confidence in the mechanistic world view had not already been undermined to a considerable extent by developments in the nineteenth century. This argument has been presented elsewhere; here I want to focus on one particular component of the revolution, the rejection of determinism, and show that there was some degree of continuity between nineteenth- and twentieth-century ideas. I do not want to overstate the case for continuity; if it were possible to quantify the causal factors responsible for the ultimate effect, I would guess that twentieth-century events (including the discovery of radioactive decay though it actually occurred just before 1900) accounted for perhaps 80% of the impetus toward atomic randomness while the nineteenth-century background accounted for the remaining 20%. That 20% is still significant in view of the fact that most historians and scientists seem to give no weight at all to the role of the well-publicized debates on the statistical interpretation of thermodynanamics of the 1890's, or to the well-established use of probability methods in kinetic theory.
(ibid, p.611-12)

But some prominent physicists, who very well knew the statistical nature of the kinetic theory of gases, were convinced that the new quantum indeterminism was of a very different kind. In particular, Arthur Stanley Eddington maintained that the determinism of classical physics, which presumably included chance and probability, was gone forever.

In The Nature of the Physical World (1928), Eddington dramatically announced "It is a consequence of the advent of the quantum theory that physics is no longer pledged to a scheme of deterministic law,"

Most mathematicians who specialized in probability (e.g., Abraham de Moivre and Pierre-Simon Laplace) believed that chance was only epistemic, the result of human ignorance. Indeed, the fact that the laws of error and the normal distribution of chance events followed precise statistical laws in the limit of large numbers of events, was for them proof that an unknown deterministic law governed all events.

Brush notes that one could easily argue that Maxwell, Boltzmann, Planck, and Einstein, would also "find it inconceivable that anything in nature could happen 'by chance' without any cause at all."

Hence whenever we find them using the words "probability," "chance," "statistical," or "spontaneous," we must assume that such terms only refer to our lack of knowledge of causes, not to the absence of causes. The fallacy of that interpretation is that it could apply equally well to Born and Heisenberg, or to anyone who believes in an "uncertainty principle" as distinct from an "indeterminacy principle."
(ibid, p.626)

Heisenberg himself emphasized that his principle applies to our knowledge about the world, The assertion that quantum mechanics has abandoned causality means that in the proposition "If we know the present exactly we can predict the future" it is not only the conclusion but also the premise that is false, according to Heisenberg:

One might be led to the conjecture that under the perceptible statistical world there is hidden a "real" world in which the causal law holds. But it seems to us that such speculations, we emphasize explicitly, are fruitless and meaningless. Physics should only describe formally the relations of perceptions....
Clearly the transition from determinism to indeterminism is linked with the positivistic-pragmatic-operationalist-instrumentalist-phenomenalist attitude that many physicists adopted in the early twentieth century, partly influenced by Ernst Mach and other critics of nineteenth-century mechanism, partly as a result of the difficulty of fitting the new phenomena of atomic physics into any consistent theoretical scheme. Positivism (as I call this complex of views) is a retreat from the aspiration to know and understand everything, an admonition to be content with the partial knowledge that can be attained at a particular stage in the development of theory and experiment. A positivist may call himself an indeterminist, meaning that his science cannot determine that which lies beyond present observation; indeterminism is then the same as "uncertainty." (This was the position of Bohr, Heisenberg, and Eddington.) Or he may call himself a determinist, meaning that his theory correlates all known or knowable facts about the observable world, and that anything beyond that is not his concern anyway. (It is in this sense that Planck and some modern physicists and philosophers say that quantum mechanics is a deterministic theory.) Conversely, an anti-positivist or realist maybe a determinist in the Laplacian sense, or an indeterminist who insists that there is a fundamental randomness in nature. Since this last position is rather hard to defend, the acceptance of indeterminism was greatly facilitated by the (at least temporary) acceptance of positivism.

Yet the acceptance of indeterminism could not have occurred unless determinism had first been shown to be either untenable or inconvenient in scientific work, since positivism is not ordinarily a very attractive stance for physicists. The contribution of nineteenth-century statistical physics was to show that in many cases the use of deterministic laws is not convenient in dealing with systems of many particles even though the motion of one or two such particles can be completely determined. Developments in the first two decades of the twentieth century showed that statistical physics can also deal with systems whose behavior does not seem to be determined by known causes. The positivistic attitude allowed the question of ultimate determinism to be set aside even as it encouraged the pragmatic use of statistical methods that carried the flavor of indeterminism.
(ibid, p.626-27)

There is perhaps more continuity between the nineteenth-century thinkers on probability and prominent dissenters from quantum theory such as Max Planck, Albert Einstein, Louis de Broglie, Erwin Schodinger, and David Bohm, who always hoped that an underlying deterministic explanation would be found some day for quantum randomness.

In his later History of Modern Science, Brush summarized these arguments about the origin of indeterminism and chance in physics dating back to about 1800.

Just as Darwin denied that he was postulating randomness as a basic principle in evolution even though his theory of natural selection seemed to provide no alternative to the assumption that variations occur by chance, Einstein supplied the basis for indeterminism in physics yet insisted that "God does not play dice." In a third paper published in 1905, Einstein treated the irregular motion of microscopic particles in a fluid ("Brownian movement") as a random process dependent on chance impacts of molecules. Eleven years later he presented a theory of spontaneous and stimulated emission of radiation — a theory that ultimately inspired the invention of the laser — in which he assumed that atomic processes are governed by chance. While Einstein himself was unhappy with this assumption, other physicists made it the basis of the quantum theory of the atom.

Randomness or indeterminism, another major theme of the Second Scientific Revolution, did not originate in quantum theory but emerged in nineteenth-century debates about the temporal direction of irreversible processes. Kelvin had proposed in 1852 a "universal tendency in nature to the dissipation of mechanical energy"; this became associated with the second law of thermodynamics, as the statement that "entropy" always increases or remains constant. (Entropy was originally defined as heat transfer divided by temperature.) Maxwell recognized that the natural tendency of heat to flow from hot to cold — the simplest example of energy dissipation or entropy increase — is equivalent to a tendency for molecules to become more and more mixed up as time goes on. Ludwig Boltzmann quantified this insight with a mathematical relation between entropy and disorder and reformulated the kinetic theory of gases so as to imply that all natural processes involve some degree of randomness at the atomic level.

Entropy was thereby liberated from its moorings in physics and entered common language as a synonym for randomness. In the twentieth century we no longer fear randomness as a threat of chaos but welcome it as a possible haven for free will and a guarantee of "fairness" in statistical surveys and military draft selection procedures.

In "quantum mechanics" (the mature version of quantum theory). randomness reached new heights of abstraction as mechanism retreated. Erwin Schrödinger proposed a mathematical equation from which can be deduced the observable properties of atoms, molecules, and (with a powerful enough computer or accurate approximate methods) any material system under ordinary conditions. But the symbols in the Schrödinger equation have no direct physical meaning. According to Max Born one of these symbols, the "wave function," represents the probability that the system will follow a certain path or be found in a certain state. There is no longer a causal law to determine how the positions and velocities of atoms evolve; instead there is a causal law that determines how their probability distributions evolve.

Following the publication in 1926 of Schrodinger's equation and Max Born's statistical interpretation of it, there ensued a friendly but intense debate between Einstein and Niels Bohr, the philosophical leader of the new quantum mechanicians. The major issue was not so much randomness as realism. Einstein argued that quantum mechanics is not wrong but incomplete because it fails to account for some atomic properties that have a real existence. For example, according to Werner Heisenberg's principle, the position and momentum of a particle cannot be simultaneously determined: the more accurately one of these quantities is pinned down, the more indeterminate the other must be. To call this an "uncertainty principle" as is usually done implies that the position and momentum actually have values but we can't find out what they are because any attempt to measure them must disturb the system. But Bohr and Heisenberg, the proponents of the "Copenhagen interpretation" of quantum mechanics, claimed that these properties cannot be said to have an objective existence. It is only the observation that gives them reality. Thus the term "indeterminacy principle" is more accurate.
(The History of Modern Science, Iowa State University Press, 1988, pp.19-20)

Brush is quite right that indeterminacy is preferable to uncertainty, with the latter's epistemic implications. But the hope that randomness is now welcome as a possible haven for free will was shared by just a few quantum scientists. Philosophers have rejected indeterminism as one of the two horns of a dilemma. For them, chance as the direct cause of human action undermines moral responsibility. Indeterminism is part of the standard argument against free will

We argue that it takes a two-stage process of randomness followed by adequate determinism to provide a workable free will model.

For Teachers
For Scholars

Chapter 1.5 - The Philosophers Chapter 2.1 - The Problem of Knowledge
Home Part Two - Knowledge
Normal | Teacher | Scholar