Citation for this page in APA citation style.           Close


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
John Dewey
Richard Double
Fred Dretske
Curt Ducasse
John Earman
Laura Waddell Ekstrom
Epictetus
Epicurus
Austin Farrer
Herbert Feigl
Arthur Fine
John Martin Fischer
Kuno 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
Gualtiero Piccinini
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

Emily Adlam
David Albert
Philip W. Anderson
Michael Arbib
Bobby Azarian
Walter Baade
Bernard Baars
Jeffrey Bada
Guido Bacciagaluppi
Leslie Ballentine
Marcello Barbieri
Jacob Barandes
Julian Barbour
Horace Barlow
Gregory Bateson
Jakob Bekenstein
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 Cavalcanti
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
Jon Jarrett
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
Markus P. 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
Antony Valentini
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

ABCD Harvard (ppt) Bhaktivedanta Institute
Biosemiotics
Free Will
Mental Causation
James Symposium
CCS25 Talk
Evo Devo September 12
Evo Devo October 2
Evo Devo Davies Nov12

 
Jon P. Jarrett

Jon Jarrett earned his Ph.D. in Philosophy at the University of Chicago in 1983. His thesis was on Bell's Theorem, Quantum Mechanics, and Local Realism.

In his thesis, Jarrett uses David Mermin's "contraption," which Mermin claims contains the essential facts of a "Bell-test" experiment. Jarrett assumes it is the logical equivalent of a physical experiment and he does a logical analysis of Bell's theorem, defining concepts with logical expressions following Mermin's suggested conventions for mathematical notations.

In 1984, Jarrett gave a talk at Harvard, and was a guest at the Center for Einstein Studies and the Center for the History and Philosophy of Science at Boston University.

In meetings that included, among others, Abner Shimony and Don Howard, Jarrett introduced a number of new technical terms that have become a major part of philosophical discussions of entanglement.

In most cases, Jarrett uses terms already well defined in physics, like "determinism," "conservation," "locality," and "completeness."

In his 1987 article on the "implications" of Bell's Theorem, Jarrett gives these terms new meanings. He calls these newly defined concepts "constraints" or "conditions" and he assembles combinations of the constraints into what he calls "claims" in a "logical 'road map' of results related to Bell's theorem."

Jarrett writes...

Any empirical theory governing the operation of the Mermin contraption must ascribe states to the measuring devices and the source emissions which (presumably by way of appropriate physical laws) functions of the form pABλ (x,y | i,j) where λ is the state of the source emissions (the pair of particles); x and y are the measurement outcomes(red or green) at A and B respectively; and i and j are respectively the A and B detector states, including the switch settings and whatever else may be relevant...I will call these pAB functions the "elementary joint probability" functions.

Determinism, for present purposes, is just the requirement that the theory specify probabilities of 0 or 1 for all possible outcomes of all possible Mermin contraption measurements.

Jarrett thus defines what he calls the constraint "DETERMINISM" not as the familiar philosophical idea that every event or state of affairs, including every human decision and action, is the inevitable and necessary consequence of antecedent states of affairs, a chain of causes and event, with one possible future.

Instead, Jarrett defines determinism as the fact that the measurement outcomes of a Bell test is limited to two possible values 0 and 1.

Using Mermin's notation, where P is probability, i and j are the inputs/switches of the Mermin contraption at A and B, and x and y are the measurement outcomes, which are "determined" to be 0 or 1, Jarrett defines what he calls a DETERMINISM "constraint" in Mermin notation...

pABλ (x,y | i,j) ≤ |0,1|

Jarrett similarly defines new constraints for the terms "CONSERVATION," "LOCALITY," and "COMPLETENESS." And he adds a new version of locality that he calls "STRONG LOCALITY," declaring it to be a "Bell-type Inequality."

Jarrett defines a constraint he calls CONSERVATION, noting that it is not the physical conservation of angular momentum

The conservation condition (or "constraint?") derives its name from the quantum-theoretic analysis of these experiments, wherein it expresses the conservation of angular momentum. This quantum-theoretic analysis is not, however, to be assumed in any of what follows. Instead, I tentatively offer as warrant for this condition (subject to a qualification to be mentioned later) this simple empirical fact: In the data of Mermin contraption experiments, in each trial in which the A and B switch settings are the same, the lights which come on at A and B agree in color. Hence for the time being, conservation is put forward as a necessary condition for empirical adequacy.

Here Jarrett's constraint has become a "condition." And he says the condition is necessary, a logical concept with little connection to empirical facts.

An empirical fact of great importance is that the outcomes of Bohm-version EPR experiments are always perfectly correlated, in opposite spin directions with a 50-50 chance of particle 1 being spin-up and particle 2 spin-down, or vice versa.

The Bohm version of EPR starts with a hydrogen molecule in a spherically symmetric "singlet" state, with total spin angular momentum zero, which disassociates into two hydrogen atoms. Bohm-EPR is describable by a two-particle wave function we can call ψ12 which is the linear combination of two terms, each the product of two single-particle wave functions, ψ1 and ψ2.

ψ12 = 1/√2(ψ1ψ2) - 1/√2(ψ2ψ1)

The coefficients 1/√2, when squared, tell us there is a 50-50 chance of finding the separated atoms in ψ1ψ2 or in ψ2ψ1. In either case the atomic spins are always found in opposite directions, when measurements are made in the same direction, preserving the symmetry, and conserving the total spin angular momentum as zero, the same as the original molecule.

It is this physical fact that led Bohm in 1951 to write...

Suppose that we have a molecule containing two atoms in a state in which the total spin is zero and that the spin of each atom is ℏ/2. Roughly speaking, this means that the spin of each atom points in a direction exactly opposite to that of the other, insofar as the spin may be said to have any definite direction at all. [Indeed, we can only say that the total spin zero of the two atoms means that their two-particle wave function ψ12 is spherically symmetric with no preferred direction - the singlet state.] Now suppose that the molecule is disintegrated by some process that does not change the total angular momentum. The two atoms will begin to separate and will soon cease to interact appreciably. [But Erwin Schrödinger tells us that they will not become independent and "cease to interact" until some measurement disentangles them, decohering their phases, and allowing their two-particle wave function ψ12 to be replaced with the product of two single-particle wave functions ψ12ψ2 or ψ2ψ1.] Their combined spin angular momentum, however, remains equal to zero, because no torques have acted on the system...

Suppose now that one measures the spin angular momentum ofany one of the particles, say No.1. Because of the existence of correlations we can immediately conclude that the angular momentum vector of the other particle (No.2) is equal and opposite to that on No.1. In this way, we can indirectly measure the angular momentum of particle No.2 by measuring the corresponding vector of particle No.1.

Bohm and Aharonov say the equivalent in 1957

Then, because the total spin is still zero, it can immediately be concluded that the same component of the spin of the other particle (B) is opposite to that of A.

Finally Bell in 1964 says...

With the example advocated by Bohm and Aharonov, the EPR argument is the following. Consider a pair of spin one-half particles formed somehow in the singlet spin state and moving freely in opposite directions. Measurements can be made, say by Stern-Gerlach magnets, on selected components of the spins σ1 and σ2. If measurement of the component σ1a, where a is some unit vector, yields the value + 1 then, according to quantum mechanics, measurement of σ2a must yield the value — 1 and vice versa.

Now why, we may ask, did not Bohm, or Bell, or modern commentators on Bell's theorem, like Jarrett, consider the conservation of total spin angular momentum zero as a "common cause" explaining the perfect measurement correlations? The conservation is true at all times for the "separating" particles up to the moment of measurements (It is known as a "quasi-molecule" because it is described with a molecular wave function and not the product of two atomic wave functions). Conservation will remain true as long as the forces involved in Stern-Gerlach spin measurements are symmetric, the two SG devices oriented in the same plane to preserve the symmetry. When the devices measure in planes at an angle to one another, the correlations fall off as the cosine squared of that angle (Malus's law).

This "common cause" is just a shared/joint property of the two particles, true at all times, not just for measurements. It is not one particle's measurement acting (instantaneously at a distance) on the other particle.

The constant total spin zero is thus a "constant of the motion." Since it achieves the goal of hypothetical "local hidden variables" traveling with the particles, we might call it a "hidden" constant of the motion.

Jarrett's Influence
Jarrett's early work had a great influence on later analyses of Bell's theorem, especially by philosophers of science, who think that logical analyses or conceptual analyses with words (analytic philosophy) can solve physical problems.

Some of these philosophers of science, starting with Jarrett himself, simply redefine "Bell's locality," claiming it contains more than simple "locality." Some also redefined "locality." Again following Jarrett, many decided that Bell's theorem and his "locality" can not be understood without understanding other complicated phenomena, such as Einstein's "realism," Bohr's "completeness," Bohm's "hidden variables," and of course philosophical "determinism."

The mathematical derivation of Bell's theorem and its meaning is not easily seen. But Bell's stated goal was to find an explanation for Einstein's "spooky action at a distance" as close as possible to Einstein's idea of "realism."

So instead of suggesting new terminology for future philosophical debates, we propose reviewing Einstein's own insights into

  1. nonlocal behavior between a particle and its single-particle wave function, between 1905 and 1927
  2. nonlocal behavior between two particles and their two-particle wave function ψ12, starting in 1933
  3. his "separability principle" (Trennungsprinzip), starting with EPR in 1935, about which,
  4. Erwin Schrödinger in his 1935 reply to EPR, told Einstein that the particles are "entangled," that is, they are not separable, until some disturbance or some measurement "disentangles" the two-particle wave function ψ12 into the product of two single-particle wave functions, either ψ1ψ2 or ψ2ψ1, after which they are separated and no longer influence one another.
  5. However, Schrödinger said, measurements of one particle may still reveal properties of the separated particle, using conservation laws.

Don Howard, who follows Jarrett's thinking and new terminology in many ways, also gave us the clearest history of Einstein's nonlocality and his nonseparability.

We should compare Jarrett's constraints, claims, and logical map with the central physical issues of quantum entanglement.

COMPLETENESS, LOCALITY, and STRONG LOCALITY

References
Jarrett, J. (1983) BELL'S THEOREM, QUANTUM MECHANICS, AND LOCAL REALISM, Ph.D. thesis. Univ. Chicago
Jarrett, J. (1984) "On the Physical Significance of the Locality Conditions in the Bell Arguments", Noùs, Vol. 18, No. 4, Special Issue on the Foundations of Quantum Mechanics, pp. 569-589
Jarrett, J. (1987) Bell's Theorem, A Guide to the Implications, in Philosophical Consequences of Quantum Theory,, James T. Cushing and Edwin McMullin, (eds.), U. Notre Dame Press.
Jarrett, J. (2009) "On the Separability of Physical Systems," in W.C. Myrvold and J. Christian (eds.), Quantum Reality, Relativistic Causality, and Closing the Epistemic Circle, The Western Ontario Series in Philosophy of Science 73,
Norsen, T. (2008) Local Causality and Completeness: Bell vs. Jarrett, arXiv
Shimony, A. (2004) Bell's Theorem, Stanford Encyclopedia of Philosophy.
Normal | Teacher | Scholar