John Archibald Wheeler

From Wikipedia, the free encyclopedia
  (Redirected from John A. Wheeler)
Jump to: navigation, search
John Archibald Wheeler
John Archibald Wheeler1985.jpg
John Archibald Wheeler ( right ) together with Eckehard W. Mielke in front of lake in Holstein before the Hermann Weyl-Conference 1985 in Kiel, Germany
Born (1911-07-09)July 9, 1911
Jacksonville, Florida, United States
Died April 13, 2008(2008-04-13) (aged 96)
Hightstown, New Jersey, United States
Residence United States
Nationality American
Fields Physics
Institutions University of North Carolina
Princeton University
University of Texas at Austin
Alma mater Johns Hopkins University (Ph.D)
Doctoral advisor Karl Herzfeld
Doctoral students Katharine Way
Hugh Everett
Richard Feynman
Bahram Mashhoon
James Griffin
Demetrios Christodoulou
Claudio Bunster
Jacob Bekenstein
Robert Geroch
John R. Klauder
Kenneth W. Ford
Charles Misner
Kip Thorne
Arthur Wightman
Bill Unruh
Robert Wald
Milton Plesset
Benjamin Schumacher
Ignazio Ciufolini
Known for Breit–Wheeler process
Wheeler–DeWitt equation
Popularizing the term "black hole"
Nuclear fission
Geometrodynamics
General relativity
Unified field theory
Wheeler–Feynman absorber theory
Wheeler's delayed choice experiment
Notable awards Albert Einstein Award (1965)
Enrico Fermi Award (1968)
Franklin Medal (1969)
National Medal of Science (1970)
Oersted Medal (1983)
Albert Einstein Medal (1988)
Matteucci Medal (1993)
Wolf Prize in Physics (1997)
Einstein Prize (APS) (2003)

John Archibald Wheeler (July 9, 1911 – April 13, 2008) was an American theoretical physicist. He was largely responsible for reviving interest in general relativity in the United States after World War II. Wheeler also worked with Niels Bohr in explaining the basic principles behind nuclear fission. One of the later collaborators of Albert Einstein, he tried to achieve Einstein's vision of a unified field theory. Together with Gregory Breit, Wheeler developed the concept of Breit–Wheeler process. He is also known for popularizing the term "black hole", for coining the terms "neutron moderator", "quantum foam", "wormhole", and "it from bit", and for hypothesizing the "one-electron universe".

Wheeler earned his doctorate at Johns Hopkins University under the supervision of Karl Herzfeld, and studied under Breit and Bohr on a National Research Council fellowship. For most of his career, Wheeler was a professor at Princeton University, which he joined in 1938, remaining until his retirement in 1976. He was influential in mentoring a generation of physicists of the Golden Age of General Relativity, who made notable contributions to quantum mechanics and gravitation. At Princeton he supervised 46 PhDs, more than any other professor in the Princeton physics department.

Wheeler teamed up with Bohr in 1939 to write a series of papers using the liquid drop model to explain the mechanism of fission. During World War II, he worked with the Manhattan Project's Metallurgical Laboratory in Chicago, where he helped design nuclear reactors, and then at the Hanford Site in Richland, Washington, where he helped DuPont build them. He returned to Princeton after the war ended, but returned to government service to help design and build the hydrogen bomb in the early 1950s.

Early life[edit]

John Archibald Wheeler was born in Jacksonville, Florida on July 11, 1911, to librarians Joseph Lewis Wheeler and Mabel Archibald (Archie) Wheeler.[1] He was the oldest of four children, with younger brothers Joseph and Robert, and a younger sister, Mary. Joseph earned Ph.D. from Brown University and a Master of Library Science from Columbia University. Robert earned a Ph.D. in geology from Harvard University, and worked as a geologist for oil companies and at colleges. Mary studied library science at the University of Denver and became a librarian.[2] They grew up in Youngstown, Ohio, but spent a year in 1921 to 1922 on a farm in Benson, Vermont, where Wheeler attended a one-room school. After they returned to Youngstown he attended Rayen High School.[3]

After graduating from the Baltimore City College high school in 1926,[4] Wheeler entered Johns Hopkins University with a scholarship from the state of Maryland.[5] He published his first scientific paper in 1930, as part of a summer job at the National Bureau of Standards.[6] He earned his doctorate in 1933. His dissertation research work, carried out under the supervision of Karl Herzfeld, was on the "Theory of the Dispersion and Absorption of Helium".[7] He received a National Research Council fellowship, which he used to study under Gregory Breit at New York University in 1933 and 1934,[8] and then in Copenhagen under Niels Bohr in 1934 and 1935.[9] In a 1934 paper, Breit and Wheeler introduced the Breit–Wheeler process, a mechanism by which photons can be potentially transformed into matter in the form of electron-positron pairs.[5][10]

In 1933, Wheeler began seeing Janette Hegner, who was taking graduate courses in history at Johns Hopkins.[11] Their relationship continued in New York the following year, after she began teaching at Rye Country Day School. They became engaged on their third date, but agreed to defer marriage until after he returned from Europe. They were married on June 10, 1935, five days after his return.[12] They had three children: Letitia, James English and Alison Wheeler.[13] Jobs were hard to come by during the Great Depression, but Arthur Ruark offered him a position as an assistant professor at the University of North Carolina at Chapel Hill, at an annual salary of $2,300, which was less than the $2,400 Janette was offered to stay at Rye Country Day School.[14][15]

Early career[edit]

Chapel Hill made Wheeler an associate professor in 1937, but he wanted to be able work more closely with the experts in particle physics. [16] He turned down an offer in 1938 of an associate professorship at Johns Hopkins University in favor of an assistant professorship at Princeton University. Although it was a lesser position, he felt that Princeton, which was building up its physics department, was a better career choice.[15] He remained a member of the faculty there until 1976.[13]

In a 1937 paper "On the Mathematical Description of Light Nuclei by the Method of Resonating Group Structure", Wheeler introduced the S-matrix – short for scattering matrix – "a unitary matrix of coefficients connecting the asymptotic behavior of an arbitrary particular solution [of the integral equations] with that of solutions of a standard form."[17][18] Heisenberg developed the idea of the S-matrix in the 1940s. Due to the problematic divergences present in quantum field theory at that time, Heisenberg was motivated to isolate the essential features of the theory that would not be affected by future changes as the theory developed. In doing so he was led to introduce a unitary "characteristic" S-matrix, which became an important tool in particle physics.[17]

Wheeler did not develop the S-matrix, but joined Edward Teller in examining Bohr's liquid drop model of the atomic nucleus.[19] They presented their results at a meeting of the American Physical Society in New York in 1938. Wheeler's Chapel Hill graduate student Katharine Way also presented a paper, which she followed up in a subsequent article, detailing how the liquid drop model was unstable under certain conditions. Due to a limitation of the liquid drop model, they all missed the opportunity to predict nuclear fission. [20][21] The news Lise Meitner and Otto Frisch's of the discovery of fission was brought to America by Bohr in 1939. Bohr told Leon Rosenfeld, who informed Wheeler.[15]

Bohr and Wheeler set to work applying the liquid drop model to explain the mechanism of nuclear fission.[22] As the experimental physicists studied fission, they uncovered puzzling results. George Placzek pointedly asked Bohr why uranium seemed to fission with both very fast and very slow neutrons. Walking to a meeting with Wheeler, Bohr had an insight: that the fission at low energies was due to the uranium-235 isotope, while at high energies it was mainly due to the far more abundant uranium-238 isotope.[23] They co-wrote two more papers on fission.[24][25] Their first paper paper appeared in the Physical Review on September 1, 1939, the day Germany invaded Poland, starting World War II in Europe.[26]

One of Wheeler's most unusual ideas came to him in 1940. Considering the idea that positrons were just electrons that were travelling backwards in time, he came up with his one-electron universe postulate: that there was in fact only electron, bouncing back and forth in time. His graduate student, Richard Feynman, found the idea hard to believe; but the idea that positrons were electrons travelling backwards in time intrigued him, and Feynman incorporated the notion of the reversibility of time into his Feynman diagrams.[27]

Nuclear weapons[edit]

Manhattan Project[edit]

Soon after the Japanese bombing of Pearl Harbor brought the United States into the war, Wheeler accepted a request from Arthur Compton to join the Manhattan Project's Metallurgical Laboratory in Chicago. He moved there in January 1942,[26] joining Eugene Wigner's group, which was studying nuclear reactor design.[28] He co-wrote a paper with Robert F. Christy on "Chain Reaction of Pure Fissionable Materials in Solution" – important in the plutonium purification process.[29] It would not be declassified until December 1955.[30] He gave the neutron moderator its name, replacing the term "slower downer" used by Enrico Fermi.[31][32]

Loading tubes of the Hanford B Reactor

After the United States Army Corps of Engineers took over the Manhattan Project, it gave responsibility for the detailed design and construction of the reactors to DuPont.[33] Wheeler became part of the DuPont design staff.[34] He worked closely with its engineers, commuting between Chicago and Wilmington, Delaware, where DuPont had its headquarters. He moved his family there in March 1943.[35] DuPont's task was not just to build nuclear reactors, but an entire plutonium production complex at the Hanford Site in Washington.[36] As work progressed, Wheeler relocated his family again in July 1944, this time to Richland, Washington, where he worked in the scientific buildings known as the 300 area.[29][35]

Even before the Hanford Site started up the B Reactor, the first of its three reactors, on September 15, 1944, Wheeler had been concerned that some nuclear fission products might turn out to be nuclear poisons, the accumulation of which would impede the ongoing nuclear chain reaction by absorbing many of the thermal neutrons that were needed to continue a chain reaction.[37] In an April 1942 report, he predicted that this would reduce the reactivity by less than one percent so long as no fission product had a neutron capture cross section of more than 100,000 barns.[38] After the reactor unexpectedly shut down, and then just as unexpectedly restarted about fifteen hours later, he suspected iodine-135, with a half life of 6.6 hours, and its daughter product, xenon-135, which has a half life of 9.2 hours. Unfortunately, xenon-135 turned out to have a neutron capture cross-section of well over 2 million barns. The problem was corrected by adding additional fuel rods to burn out the poison.[39]

Wheeler had a personal reason for working on the Manhattan Project. His brother Joe, fighting in Italy, sent him a postcard with a simple message: "Hurry up".[40] It was already too late: Joe was killed in October 1944. "Here we were," Wheeler later wrote, "so close to creating a nuclear weapon to end the war. I couldn't stop thinking then, and haven't stopped thinking since, that the war could have been over in October 1944."[39] Joe left a widow and baby daughter, Mary Jo, who later married physicist James Hartle.[41]

Hydrogen bomb[edit]

In August 1945, Wheeler and his family returned to Princeton, where he resumed his academic career.[42] Working with Feynman, he explored the possibility of physics with particles, but not fields, and he carried out theoretical studies of the muon with Jayme Tiomno,[43] resulting in a series of papers on the topic,[44][45] including a 1949 paper in which Tiomno and Wheeler introduced the "Tiomno Triangle", which related different forms of radioactive decay.[46] He also suggested the use of muons as a nuclear probe.[47] This paper, written in 1949 but not published in 1953, resulted in a series of measurements of the Chang radiation emitted by muons. Muons are a component of cosmic rays, and Wheeler became the founder and first director of Princeton's Cosmic Rays Laboratory, which received a substantial grant of $375,000 from the Office of Naval Research in 1948.[48] He received a Guggenheim Fellowship in 1946,[49] which allowed him to spend the 1949–50 academic year in Paris.[50]

The "Sausage" device of Ivy Mike nuclear test on Enewetak Atoll. The Sausage was the first true hydrogen bomb ever tested.

The 1949 detonation of Joe-1 by the Soviet Union prompted an all-out effort by the United States to develop the more powerful hydrogen bomb in response, led by Teller. Henry D. Smyth, Wheeler's department head at Princeton, asked him to join the effort. Most physicists were, like Wheeler, trying to re-establish careers interrupted by the war, and were reluctant to face more disruption. Others had moral objections.[51] Ones who agreed to participate included Emil Konopinski, Marshall Rosenbluth, Lothar Nordheim and Charles Critchfield; but there was also now a body of experienced weapons physicists at the Los Alamos Laboratory, led by Norris Bradbury.[52][53] Wheeler agreed to go to Los Alamos after a conversation with Bohr.[51] Two of his graduate students from Princeton, Ken Ford and John Toll, joined him there.[54]

At Los Alamos, Wheeler and his family moved into the house on "Bathtub Row" that had been occupied by Robert Oppenheimer and his family during the war.[55] In 1950, there was no practical design for a hydrogen bomb. Calculations by Stan Ulam and others showed that Teller's "Classical Super" would not work. Teller and Wheeler created a new design known as "Alarm Clock", but it was not a true thermonuclear weapon. Not until January 1951 did Ulam come up with a workable design.[56]

In 1951, Wheeler obtained permission from Bradbury to set up a branch office of the Los Alamos laboratory at Princeton, known as Project Matterhorn. It had two parts. Matterhorn S (for stellarator, another name coined by Wheeler), under Lyman Spitzer, investigated nuclear fusion as a power source. Matterhorn B (for bomb), under Wheeler, engaged in nuclear weapons research. Senior scientists still remained disinterested and aloof from the project, so he staffed it with young graduate and post-doctoral students.[57] In January 1953, he was involved in a security breach when he lost a highly classified paper on lithium-6 and the hydrogen bomb design during an overnight train trip. This resulted in Wheeler being given him an official reprimand. [58] Matterhorn B's efforts were crowned by the success of the Ivy Mike nuclear test at Enewetak Atoll in the Pacific, on November 1, 1953,[59][57] which Wheeler witnessed. The yield of the Ivy Mike "Sausage" device was reckoned at 10.4 megatons of TNT (44 PJ), about 30 percent higher than Matterhorn B had estimated.[60] Matterhorn B was discontinued, but Matterhorn S endures, as the Princeton Plasma Physics Laboratory.[57]

Later life[edit]

Geometrodynamics[edit]

After concluding his Matterhorn Project work, Wheeler resumed his academic career. In a 1955 paper, he theoretically investigated the geon, an electromagnetic or gravitational wave which is held together in a confined region by the attraction of its own field. He coined the name as a contraction of "gravitational electromagnetic entity."[61] He found that the smallest geon was a toroid the size of the Sun, but a millions heavier.[62] While working on mathematical extensions to Einstein's Theory of General Relativity in 1957, Wheeler introduced the concept and the word wormhole to describe hypothetical "tunnels" in space-time. Bohr pointedly asked if they are stable; further research by Wheeler determined that they are not.[63][64]

During the 1950s, Wheeler formulated geometrodynamics, a program of physical and ontological reduction of every physical phenomenon, such as gravitation and electromagnetism, to the geometrical properties of a curved space-time.[65][66] Wormholes were just one manifestation of what Wheeler envisaged as the fabric of the universe, a chaotic sub-atomic realm of quantum fluctuations, which he called "quantum foam".[61][67] For a few decades, general relativity had not been considered a very respectable field of physics, being detached from experiment. Wheeler was a key figure in the revival of the subject, leading the school at Princeton, while Sciama and Zel'dovich developed the subject at Cambridge University and the University of Moscow. The work of Wheeler and his students made high contributions to the Golden Age of General Relativity.[68] His work in general relativity included the theory of gravitational collapse. He used the term black hole in 1967 during a talk he gave at the NASA Goddard Institute of Space Studies (GISS).[69] He was also a pioneer in the field of quantum gravity with his development with Bryce DeWitt of the Wheeler–DeWitt equation,[70] which is the equation governing the "wave function of the Universe".[71]

Quantum[edit]

Illustration of a black hole and its surrounding disk

Recognizing Wheeler's colorful way with words, characterized by such confections as "mass without mass", the festschrift honoring his 60th birthday was fittingly entitled Magic Without Magic: John Archibald Wheeler: A Collection of Essays in Honor of his Sixtieth Birthday (1972). That same writing style could also attract parodies, including a famous one by "John Archibald Wyler" that was affectionately published by a relativity journal.[72][73] Wheeler wrote Geometrodynamuics (1962), and teamed up with Edwin F. Taylor to write Spacetime Physics (1966) and Scouting Black Holes (1996). With Kent Harrison, Kip Thorne and Masami Wakano he wrote Gravitation Theory and Garvitional Collapse (1954). This led to the voluminous general relativity textbook Gravitation (1973), co-written with Misner and Thorne. Its timely appearance during the golden age of general relativity and its comprehensiveness made it an influential relativity textbook for a generation.[74]

Wheeler retired from Princeton University in 1976, at the age of 65. He was the director of the Center for Theoretical Physics at the University of Texas at Austin from 1976 until 1986, when he retired,[13] and became a professor emeritus there.[75] Misner, Thorne and Wojciech Zurek, all former students of Wheeler, wrote that:

Looking back on Wheeler’s 10 years at Texas, many quantum information scientists now regard him, along with IBM’s Rolf Landauer, as a grandfather of their field. That, however, was not because Wheeler produced seminal re-search papers on quantum information. He did not—with one major exception, his delayed-choice experiment. Rather, his role was to inspire by asking deep questions from a radical conservative viewpoint and, through his questions, to stimulate others’ research and discovery.[76]

Wheeler's delayed choice experiment is actually several thought experiments in quantum physics, that he proposed, with the most prominent among them appearing in 1978 and 1984. These experiments are attempts to decide whether light somehow "senses" the experimental apparatus in the double-slit experiment it will travel through and adjusts its behavior to fit by assuming the appropriate determinate state for it, or whether light remains in an indeterminate state, neither wave nor particle, and responds to the "questions" asked of it by responding in either a wave-consistent manner or a particle-consistent manner depending on the experimental arrangements that ask these "questions".[77]

Over the years, Wheeler's graduate students included Katharine Way, Richard Feynman, David Hill, Bei-Lok Hu, Kip Thorne, Jacob Bekenstein, John R. Klauder, William Unruh, Robert M. Wald, Arthur Wightman, Charles Misner and Hugh Everett.[7][78] Unlike some scholars, Wheeler gave a high priority to teaching. Even after he became a famous physicist, he continued to teach freshman and sophomore physics, saying that the young minds were the most important. At Princeton he supervised 46 PhDs, more than any other professor in the Princeton physics department.[79]

In 1979, Wheeler spoke to the American Association for the Advancement of Science (AAAS), asking it to expel parapsychology, which had been admitted ten years earlier at the request of Margaret Mead. He called it a pseudoscience,[80] saying he did not oppose earnest research into the questions, but he thought the "air of legitimacy" of being an AAAS-Affiliate should be reserved until convincing tests of at least a few so-called psi effects could be demonstrated.[81] During his presentation Wheeler incorrectly stated that J. B. Rhine had committed fraud as a student, and was forced to retract that statement in a letter to the journal Science .[82] His request was turned down, and the Parapsychological Association remained a member of the AAAS.[81]

It from bit[edit]

In 1990, Wheeler suggested that information is fundamental to the physics of the universe. According to this "it from bit" doctrine, all things physical are information-theoretic in origin.

Wheeler: It from bit. Otherwise put, every "it" — every particle, every field of force, even the space-time continuum itself — derives its function, its meaning, its very existence entirely — even if in some contexts indirectly — from the apparatus-elicited answers to yes-or-no questions, binary choices, bits. "It from bit" symbolizes the idea that every item of the physical world has at bottom — a very deep bottom, in most instances — an immaterial source and explanation; that which we call reality arises in the last analysis from the posing of yes-or-no questions and the registering of equipment-evoked responses; in short, that all things physical are information-theoretic in origin and that this is a participatory universe.[83]

Wheeler speculated that reality is created by observers in the universe. "How does something arise from nothing?", he asked about the existence of space and time.[84] He also coined the term "Participatory Anthropic Principle" (PAP), a version of a Strong Anthropic Principle. From a transcript of a radio interview on "The anthropic universe":

Wheeler: We are participators in bringing into being not only the near and here but the far away and long ago. We are in this sense, participators in bringing about something of the universe in the distant past and if we have one explanation for what's happening in the distant past why should we need more?
Martin Redfern: Many don't agree with John Wheeler, but if he's right then we and presumably other conscious observers throughout the universe, are the creators — or at least the minds that make the universe manifest.[85]

Over the years Wheeler gathered many prizes and awards, including the Enrico Fermi Award in 1968, the Franklin Medal in 1969, the National Medal of Science in 1971, the Einstein Prize in 1969, the Niels Bohr International Gold Medal in 1982, the Oersted Medal in 1983, the J. Robert Oppenheimer Memorial Prize in 1984 and the Wolf Foundation Prize in 1997.[75] He was a member of the American Philosophical Society, the Royal Academy, the Accademia Nazionale dei Lincei, and the Century Association. He received honorary degrees from 18 different institutions, and in 2001, Princeton used a $3 million gift to establish the John Archibald Wheeler/Battelle Professorship in Physics.[13] After his death, the University of Texas named the John A. Wheeler Lecture Hall in his honor.[75]

On April 13, 2008, Wheeler died of pneumonia at the age of 96 in Hightstown, New Jersey.[86] He was survived by his three children, his wife having died in October 2007.[13]

Bibliography[edit]

  • Wheeler, John Archibald (1962). Geometrodynamics. New York: Academic Press. OCLC 1317194. 
  • Misner, Charles W.; Kip S. Thorne; John Archibald Wheeler (September 1973). Gravitation. San Francisco: W. H. Freeman. ISBN 0-7167-0344-0. 
  • Wheeler, John Archibald (1979). Some Men and Moments in the History of Nuclear Physics: The Interplay of Colleagues and Motivations. Minneapolis: University of Minnesota Press. OCLC 6025422. 
  • Wheeler, John Archibald (1990). A Journey Into Gravity and Spacetime. -Scientific American Library. New York: W.H. Freeman. ISBN 0-7167-6034-7. 
  • Wheeler, John Archibald (1992). Spacetime Physics: Introduction to Special Relativity'. New York: W. H. Freeman. ISBN 0-7167-2327-1. 
  • Wheeler, John Archibald (1994). At Home in the Universe. New York: American Institute of Physics. ISBN 1-56396-500-3. 
  • Ciufolini, Ignazio; Wheeler, John Archibald (1995). Gravitation and Inertia. Princeton, New Jersey: Princeton University Press. ISBN 0-691-03323-4. 
  • Wheeler, John Archibald (1998). Geons, Black Holes, and Quantum Foam: A Life in Physics. New York: W.W. Norton & Co. ISBN 0-393-04642-7. 
  • Wheeler, John Archibald (2000). Exploring Black Holes: Introduction to General Relativity. Addison Wesley. ISBN 0-201-38423-X. 

Notes[edit]

  1. ^ Wheeler & Ford 1998, pp. 64, 71.
  2. ^ Wheeler & Ford 1998, pp. 71–75.
  3. ^ Wheeler & Ford 1998, pp. 78–80.
  4. ^ Leonhart 1939, p. 287.
  5. ^ a b Wheeler & Ford 1998, p. 85.
  6. ^ Wheeler & Ford 1998, p. 97.
  7. ^ a b John Archibald Wheeler at the Mathematics Genealogy Project
  8. ^ Wheeler & Ford 1998, pp. 105–107.
  9. ^ Wheeler & Ford 1998, pp. 123–127.
  10. ^ Breit, G.; Wheeler, John (December 1934). "Collision of Two Light Quanta". Physical Review (American Physical Society) 46 (12): 1087–1091. doi:10.1103/PhysRev.46.1087. 
  11. ^ Wheeler & Ford 1998, p. 102.
  12. ^ Wheeler & Ford 1998, pp. 121–122.
  13. ^ a b c d e MacPherson, Kitta (April 14, 2008). "Leading physicist John Wheeler dies at age 96". News at Princeton. 
  14. ^ Wheeler & Ford 1998, pp. 144–145.
  15. ^ a b c Ford, Kenneth W. (February 4, 1994). "Interview with Dr. John Wheeler – Session VI". American Institute of Physics. 
  16. ^ Wheeler & Ford 1998, pp. 151–152.
  17. ^ a b Mehra & Rechenberg 1982, p. 990.
  18. ^ Wheeler, John A. (December 1937). "On the Mathematical Description of Light Nuclei by the Method of Resonating Group Structure". Physical Review (American Physical Society) 52 (11): 1107–1122. Bibcode:1937PhRv...52.1107W. doi:10.1103/PhysRev.52.1107. 
  19. ^ Teller, E.; Wheeler, J. A. (May 1938). "On the Rotation of the Atomic Nucleus". Physical Review (American Physical Society) 53 (10): 778–789. doi:10.1103/PhysRev.53.778. 
  20. ^ Mehra & Rechenberg 1982, pp. 990–991.
  21. ^ Way, Katharine (May 1939). "The Liquid-Drop Model and Nuclear Moments". Physical Review (American Physical Society) 55 (10): 963–965. Bibcode:1939PhRv...55..963W. doi:10.1103/PhysRev.55.963. 
  22. ^ Bohr, John Archibald; Wheeler (September 1939). "The Mechanism of Nuclear Fission". Phys. Rev. (American Physical Society) 56 (5): 426–450. doi:10.1103/PhysRev.56.426. 
  23. ^ Wheeler & Ford 1998, pp. 27–28.
  24. ^ Bohr, John Archibald; Wheeler (November 1939). "The Fission of Protactinium". Physical Review (American Physical Society) 56 (10): 1065–1066. doi:10.1103/PhysRev.56.1065.2. 
  25. ^ Bohr, John Archibald; Wheeler (January 1940). Journal of Applied Physics 11 (1): 70–71. doi:10.1063/1.1712708. ISSN 0021-8979. 
  26. ^ a b Wheeler & Ford 1998, p. 31.
  27. ^ Wheeler & Ford 1998, pp. 117–118.
  28. ^ Wheeler & Ford 1998, p. 39.
  29. ^ a b Ford, Kenneth W. (February 14, 1994). "Interview with Dr. John Wheeler – Session VII". American Institute of Physics. 
  30. ^ Christy, R. F.; Wheeler, J. A. (January 1, 1943). "Chain Reaction of Pure Fissionable Materials in Solution". Metallurgical Laboratory. 
  31. ^ Wheeler & Ford 1998, p. 40.
  32. ^ Weinberg 1994, p. 14.
  33. ^ Weinberg 1994, pp. 27–30.
  34. ^ Jones 1985, p. 203.
  35. ^ a b Wheeler & Ford 1998, pp. 46–48.
  36. ^ Jones 1985, pp. 210–211.
  37. ^ Rhodes 1986, pp. 558–60.
  38. ^ Wheeler & Ford 1998, p. 56.
  39. ^ a b Wheeler & Ford 1998, p. 61.
  40. ^ Gefter, Amanda (January 16, 2014). "Haunted by His Brother, He Revolutionized Physics". Nautilus (9). 
  41. ^ Wheeler & Ford 1998, p. 75.
  42. ^ Wheeler & Ford 1998, pp. 161–162.
  43. ^ Wheeler & Ford 1998, pp. 171–177.
  44. ^ Wheeler, John (March 1947). "Mechanism of Capture of Slow Mesons". Physical Review (American Physical Society) 71 (5): 320–321. doi:10.1103/PhysRev.71.320. 
  45. ^ Tiomno; Wheeler, J. A. (January 1949). "Charge-Exchange Reaction of the μ-Meson with the Nucleus". Reviews of Modern Physics (American Physical Society) 21 (1): 153–165. doi:10.1103/RevModPhys.21.153. 
  46. ^ Tiomno, J.; Wheeler, J. A. (January 1949). Reviews of Modern Physics 21 (1): 144–152. doi:10.1103/RevModPhys.21.144. 
  47. ^ Wheeler, John (November 1953). "Mu Meson as Nuclear Probe Particle". Physical Review (American Physical Society) 92 (3): 812–816. doi:10.1103/PhysRev.92.812. 
  48. ^ Wheeler & Ford 1998, pp. 177–179.
  49. ^ "John A. Wheeler". John Simon Guggenheim Memorial Foundation. Retrieved December 6, 2014. 
  50. ^ Wheeler & Ford 1998, p. 183.
  51. ^ a b Wheeler & Ford 1998, pp. 188–189.
  52. ^ Rhodes 1995, pp. 416–417.
  53. ^ Wheeler & Ford 1998, p. 202.
  54. ^ Wheeler & Ford 1998, pp. 193–194.
  55. ^ Wheeler & Ford 1998, p. 196.
  56. ^ Rhodes 1995, pp. 457–464.
  57. ^ a b c Wheeler & Ford 1998, pp. 218–220.
  58. ^ Wheeler & Ford 1998, pp. 285–286.
  59. ^ Ford, Kenneth W. (April 2009). "John Wheeler’s work on particles, nuclei, and weapons". Physics Today 62 (4): 29–33. doi:10.1063/1.3120893. 
  60. ^ Wheeler & Ford 1998, pp. 224–225.
  61. ^ a b Wheeler, J. A. (January 1955). "Geons". Physical Review 97 (2): 511–536. Bibcode:1955PhRv...97..511W. doi:10.1103/PhysRev.97.511. 
  62. ^ Wheeler & Ford 1998, p. 237.
  63. ^ Wheeler & Ford 1998, pp. 239–241.
  64. ^ Misner, Charles W.; Wheeler, John A. (December 1957). "Classical Physics as Geometry". Annals of Physics 2 (6): 525–603. doi:10.1016/0003-4916(57)90050-7. ISSN 0003-4916. 
  65. ^ J. Wheeler (1961). "Geometrodynamics and the Problem of Motion". Reviews of Modern Physics 44 (1): 63. Bibcode:1961RvMP...33...63W. doi:10.1103/RevModPhys.33.63. 
  66. ^ J. Wheeler (1957). "On the nature of quantum geometrodynamics". Ann. Phys. 2 (6): 604–614. Bibcode:1957AnPhy...2..604W. doi:10.1016/0003-4916(57)90050-7. 
  67. ^ Wheeler & Ford 1998, p. 248.
  68. ^ Hawking et al. 2003, pp. 80–88.
  69. ^ Wheeler & Ford 1998, p. 296.
  70. ^ DeWitt, B. S. (1967). "Quantum Theory of Gravity. I. The Canonical Theory". Phys. Rev. 160 (5): 1113–1148. Bibcode:1967PhRv..160.1113D. doi:10.1103/PhysRev.160.1113. 
  71. ^ Hartle, J.; Hawking, S. (December 1983). "Wave function of the Universe". Physical Review D (American Physical Society) 28 (12): 2960–2975. doi:10.1103/PhysRevD.28.2960. 
  72. ^ Wyler, John Archibald (1974). "Rasputin, Science, and the Transmogrification of Destiny". General Relativity and Gravitation 5 (2): 175–182. 
  73. ^ Misner 2010, p. 22.
  74. ^ Wheeler & Ford 1998, pp. 232–234.
  75. ^ a b c "Report of the Memorial Resolution Committee for John A. Wheeler". Retrieved December 6, 2014. 
  76. ^ Misner, Charles W.; Thorne, Kip S.; Zurek, Wojciech H. (April 2009). "John Wheeler, relativity, and quantum information". Physics Today 62 (4): 40–46. doi:10.1063/1.3120895. 
  77. ^ Wheeler & Ford 1998, pp. 334–339.
  78. ^ Saunders 2010, p. 6.
  79. ^ Christensen, Terry M. (April 2009). "John Wheeler’s Mentorship: An Eenduring Legacy". Physics Today 62 (4): 55–59. doi:10.1063/1.3120897. 
  80. ^ Gardner & 1981, pp. 185ff.
  81. ^ a b Wheeler & Ford 1998, pp. 342–343.
  82. ^ Wheeler, J. A. (1979). "Parapsychology – A correction". Science 205 (4402): 144. 
  83. ^ Wheeler 1990, p. 5.
  84. ^ Ford 2006, p. 2.
  85. ^ "The anthropic universe". Science Show. 18 February 2006. 
  86. ^ Overbye, Dennis (April 14, 2008). "John A. Wheeler, Physicist Who Coined the Term ‘Black Hole’, Is Dead at 96.". The New York Times. Retrieved April 15, 2008. John A. Wheeler, a visionary physicist and teacher who helped invent the theory of nuclear fission, gave black holes their name and argued about the nature of reality with Albert Einstein and Niels Bohr, died Sunday morning at his home in Hightstown, N.J. He was 96. 

References[edit]

External links[edit]