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 Belsham Henri Bergson George Berkeley Isaiah Berlin Richard J. Bernstein Bernard Berofsky Robert Bishop Max Black Susanne Bobzien Emil du BoisReymond Hilary Bok Laurence BonJour George Boole Émile Boutroux F.H.Bradley C.D.Broad Michael Burke Lawrence Cahoone C.A.Campbell Joseph Keim Campbell Rudolf Carnap Carneades 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 Herbert Feigl Arthur Fine John Martin Fischer Owen Flanagan Luciano Floridi Philippa Foot Alfred Fouilleé Harry Frankfurt Richard L. Franklin 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 William James Lord Kames Robert Kane Immanuel Kant Tomis Kapitan Jaegwon Kim William King Hilary Kornblith Christine Korsgaard Saul Kripke Andrea Lavazza Christoph Lehner Keith Lehrer Gottfried Leibniz Jules Lequyer Leucippus Michael Levin George Henry Lewes C.I.Lewis David Lewis Peter Lipton C. Lloyd Morgan John Locke Michael Lockwood E. Jonathan Lowe John R. Lucas Lucretius Alasdair MacIntyre Ruth Barcan Marcus James Martineau 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.NowellSmith 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 JeanPaul Sartre Kenneth Sayre T.M.Scanlon Moritz Schlick Arthur Schopenhauer John Searle Wilfrid Sellars Alan Sidelle Ted Sider Henry Sidgwick Walter SinnottArmstrong 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 Michael Arbib Walter Baade Bernard Baars Leslie Ballentine Gregory Bateson 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 Hans Briegel Leon Brillouin Stephen Brush Henry Thomas Buckle S. H. Burbury Donald Campbell Anthony Cashmore Eric Chaisson JeanPierre Changeux Arthur Holly Compton John Conway John Cramer E. P. Culverwell Olivier Darrigol Charles Darwin Richard Dawkins Terrence Deacon Lüder Deecke Richard Dedekind Louis de Broglie Max Delbrück Abraham de Moivre Paul Dirac Hans Driesch John Eccles Arthur Stanley Eddington Gerald Edelman Paul Ehrenfest Albert Einstein Hugh Everett, III Franz Exner Richard Feynman R. A. Fisher Joseph Fourier Philipp Frank Lila Gatlin Michael Gazzaniga GianCarlo Ghirardi J. Willard Gibbs Nicolas Gisin Paul Glimcher Thomas Gold A.O.Gomes Brian Goodwin Joshua Greene Jacques Hadamard Mark Hadley Patrick Haggard Stuart Hameroff Augustin Hamon Sam Harris Hyman Hartman JohnDylan Haynes Donald Hebb Martin Heisenberg Werner Heisenberg John Herschel Art Hobson Jesper Hoffmeyer E. T. Jaynes William Stanley Jevons Roman Jakobson Pascual Jordan Ruth E. Kastner Stuart Kauffman Martin J. Klein Simon Kochen Hans Kornhuber Stephen Kosslyn Ladislav Kovàč Leopold Kronecker Rolf Landauer Alfred Landé PierreSimon Laplace David Layzer Benjamin Libet Seth Lloyd Hendrik Lorentz Josef Loschmidt Ernst Mach Donald MacKay Henry Margenau James Clerk Maxwell Ernst Mayr John McCarthy Ulrich Mohrhoff Jacques Monod Emmy Noether Abraham Pais Howard Pattee Wolfgang Pauli Massimo Pauri Roger Penrose Steven Pinker Colin Pittendrigh Max Planck Susan Pockett Henri Poincaré Daniel Pollen Ilya Prigogine Hans Primas Adolphe Quételet Jürgen Renn/a> Juan Roederer Jerome Rothstein David Ruelle Tilman Sauer Erwin Schrödinger Aaron Schurger Claude Shannon David Shiang Herbert Simon Dean Keith Simonton B. F. Skinner Lee Smolin Roger Sperry John Stachel Henry Stapp Tom Stonier Antoine Suarez Leo Szilard Max Tegmark William Thomson (Kelvin) Giulio Tononi Peter Tse Vlatko Vedral Heinz von Foerster John von Neumann John B. Watson Daniel Wegner Steven Weinberg Paul A. Weiss John Wheeler Wilhelm Wien Norbert Wiener Eugene Wigner E. O. Wilson H. Dieter Zeh Ernst Zermelo Wojciech Zurek Konrad Zuse Fritz Zwicky Presentations Biosemiotics Free Will Mental Causation James Symposium 
Complementarity
In the late Winter of 1927, Neils Bohr went skiing for a few weeks in Norway, during which he analyzed the puzzling situation in quantum mechanics in deeply philosophical terms.
In the previous two years, Max Born, with his clever students Werner Heisenberg and Pascual Jordan, had developed the quantum mechanics of material particles. They had derived most of the results of Bohr's old quantum theory, eliminating his idea of semiclassical orbits but confirming Bohr's "quantum postulate of stationary states with electrons "jumping" between them, radiating energy with E_{2}  E_{1} = hν, following Max Planck's hypothesis about the quantum of action. And just the year before, Erwin Schrödinger developed an alternative "wave mechanics," which he showed gives exactly the same results as quantum mechanics, but without some of the major assumptions in Bohr's earlier work, which had been adopted also by Heisenberg. In his 1929 textbook, Heisenberg dubbed their work "Der Kopenhagener Geist," many years later known as the "Copenhagen interpretation" of quantum mechanics. Where Bohr and Heisenberg described the stationary states with arbitrary quantum numbers, Schrödinger showed quantum numbers emerge naturally from the number of nodes in his wave function that could fit around an electron orbit (an idea that Louis de Broglie had proposed earlier). The dualistic view that matter might consist of either particles or waves (or maybe both) must surely have inspired Bohr to think about complementary relations, but there are strong reasons to think that he might not have wanted to identify his complementarity with Einstein's ideas about "waveparticle duality". Heisenberg said that "The main point was that Bohr wanted to take this dualism between waves and corpuscles as the central point of the problem." But Bohr also used the term complementary to describe the "reciprocal uncertainty" between momentum and position in Heisenberg's indeterminacy relations. Bohr said: the measurement of the positional coordinates of a particle is accompanied not only by a finite change in the dynamical variables, but also the fixation of its position means a complete rupture in the causal description of its dynamical behaviour, while the determination of its momentum always implies a gap in the knowledge of its spatial propagation. Just this situation brings out most strikingly the complementary character of the description of atomic phenomena [italics added] Bohr may never have completely accepted Albert Einstein's idea that light itself might consist of particles, since quantum particles are complements of classical waves. In 1905, Einstein had proposed his "lightquantum hypothesis," that light came in discrete and discontinuous quantities, something like Newton's "light corpuscles." Einstein wrote in 1905:
On the modern quantum view, what spreads out is a wave of probability amplitude for absorbing a whole "light quantum" somewhere. The wave function ψ should be thought of as a "possibility" function
In accordance with the assumption to be considered here, the energy of a light ray spreading out from a point source is not continuously distributed over an increasing space but consists of a finite number of energy quanta which are localized at points in space, which move without dividing, and which can only be produced and absorbed as whole units. Bohr resisted Einstein's "lightquantum hypothesis" in 1913. His Bohr model of the atom postulated that there are "stationary states" with energy levels E_{n}. His second postulate was that electrons jump discontinuously between levels, emitting or absorbing radiation of frequency ν, where
E_{m}  E_{n} = hν
As obvious as it is today that Bohr's hν is a "photon" (as it was dubbed in the middle 1920's), Bohr thought that the radiation emitted or absorbed was continuous and classical electromagnetism. It is not clear that Bohr had completely accepted photons and the dual nature of light even as he formulated his philosophical notion of complementarity in his "Como Lecture" of 1927. He seems to have accepted it in 1949, in his tribute to Einstein. Einstein had written as early as 1909 that the wave theory of light might need to be augmented to explain his particlelike properties.
This was the beginning of waveparticle duality that Bohr would reconcile
with the idea of complementarity in quantum mechanics When light was shown to exhibit interference and diffraction, it seemed almost certain that light should be considered a wave...A large body of facts shows undeniably that light has certain fundamental properties that are better explained by Newton's emission theory of light than by the oscillation theory. For this reason, I believe that the next phase in the development of theoretical physics will bring us a theory of light that can be considered a fusion of the oscillation and emission theories... When Bohr returned from his skiing vacation, he received a draft paper from Heisenberg claiming that some physical variables might be measured precisely, but then their canonically conjugate variables would have a very large error. This is his famous "indeterminacy principle." If a momentum measurement has accuracy Δp and position accuracy Δx than the product of the two indeterminacies is Δp Δx ≥ h, where h is Planck's constant for the quantum of action. Bohr asked Heisenberg to include his notion of complementarity, and perhaps his derivation of indeterminacy from pure wavemechanical considerations, in his new paper. This upset Heisenberg greatly, because he thought that Schrödinger's "wave mechanics" added nothing to his particleoriented "matrix mechanics." Bohr thought both were needed. Though somewhat contradictory, they were his first example of "complementarity." Definitions of complementarity today almost always include waveparticle duality, but Bohr was so vague about the precise meaning of his term complementarity when he introduced it in his 1927 "Como Lecture" that it is confusing to this day. One thing he did in the Como Lecture was to argue that both Heisenberg's discontinuous and indeterministic particle picture and Schrödinger's continuous and deterministic wave picture were both needed in quantum mechanics. The theories themselves, matrix mechanics and wave mechanics, are "complementary." Almost no one, least of all Bohr, gave credit to Einstein, for his 1909 insight that both wave and particle pictures needed to be fused, or to his views in the early 1920's that the wave was a "Gespensterfeld" (ghost field) that guides the particles. Ironically, and unjustly, to this day the "Bohr atom" is taught as discontinuous "jumps" between energy levels accompanied by the emission or absorption of a photon, whereas Bohr fought against Einstein's light quantum hypothesis for decades. Einstein developed the quantum theory of radiation, explaining emission, absorption, and the radical hypothesis of "stimulated emission" (that led to the invention of the laser) in 1916! But it is Bohr's name most often cited. Bohr claimed that an experimental apparatus must always be treated as a classical object and described using ordinary language. He thought that specific experiments could reveal only part of the quantum nature of microscopic objects. For example, one experiment might reveal a particle's dynamical properties such as energy, momentum, position, etc. Another experiment might reveal wavelike properties. But no one experiment could exhaustively reveal both. The experiments needed to reveal both are "complementary." Bohr's first definition of complementarity in the Como lecture somewhat opaquely contrasts the "spacetime coordination" with the "claim of causality." And again, a few paragraphs later, Bohr looks for a complementary relation between the "kinematics" of a spacetime picture and the "dynamics" of a causal picture using variables like momentum, energy, etc. : This situation would seem clearly to indicate the impossibility of a causal spacetime description of the light phenomena. On one hand, in attempting to trace the laws of the timespatial propagation of light according to the quantum postulate, we are confined to statistical considerations. On the other hand, the fulfilment of the claim of causality for the individual light processes, characterised by the quantum of action, entails a renunciation as regards the spacetime description.Bohr points out that in expressions like ΔE Δt = h and Δp Δx = h, we see both spacetime (wave) variables x, t and dynamical (particle) variables E, p. As mentioned above, Bohr thought Heisenberg's "uncertainty" could be an example of complementarity, because two different measurement apparatuses were needed to measure dynamical momentum and spacetime position. An important contribution to the problem of a consistent application of these methods has been made lately by Heisenberg (Zeitschr. f. Phys., 43, 172; 1927). In particular, he has stressed the peculiar reciprocal uncertainty which affects all measurements of atomic quantities. Before we enter upon his results it will be advantageous to show how the complementary nature of the description appearing in this uncertainty is unavoidable already in an analysis of the most elementary concepts employed in interpreting experience. Bohr notes that Heisenberg's derivation of his indeterminacy principle was entirely done with particles and dynamical variables. Bohr then proceeds to derive Heisenberg's relations solely on the basis of a wave theory (a spacetime description). This must have embarrassed Heisenberg, who resisted at first but eventually completely accepted and promoted Bohr's view of complementarity as an essential part of the Copenhagen Interpretation (along with his own uncertainty principle and Born's statistical interpretation of the wave function).
To summarize, Bohr saw many elements of the new quantum mechanics as revealing his deep insight into complementarity. Among them were:
In later years Bohr came to think that complementarity was important in philosophy and many other fields:
For Teachers
For Scholars
Key Components of Complementarity
