John Archibald Wheeler

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John Archibald Wheeler
Wheeler in 1985
Born(1911-07-09)July 9, 1911
DiedApril 13, 2008(2008-04-13) (aged 96)
EducationJohns Hopkins University (BS, MS, PhD)
Known for
SpouseJanette Hegner
Awards
Scientific career
FieldsPhysics
Institutions
ThesisTheory of the dispersion and absorption of helium (1933)
Doctoral advisorKarl Herzfeld
Doctoral students
See list

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 to explain the basic principles of nuclear fission. Together with Gregory Breit, Wheeler developed the concept of the Breit–Wheeler process. He is best known for popularizing the term "black hole"[1] for objects with gravitational collapse already predicted during the early 20th century, for inventing the terms "quantum foam", "neutron moderator", "wormhole" and "it from bit",[2] and for hypothesizing the "one-electron universe". Stephen Hawking called Wheeler the "hero of the black hole story".[3]

At 21, Wheeler earned his doctorate at

hydrogen bomb in the early 1950s. He and Edward Teller were the main civilian proponents of thermonuclear weapons.[4]

For most of his career, Wheeler was a professor of physics at Princeton University, which he joined in 1938, remaining until 1976. At Princeton he supervised 46 PhD students, more than any other physics professor.

Wheeler left Princeton at the age of 65. He was appointed director of the Center for Theoretical Physics at the

professor emeritus
.

Early life and education

Wheeler was born in

Master of Library Science from Columbia University. His brother Robert earned a PhD in geology from Harvard University and worked as a geologist for oil companies and several colleges. His sister Mary studied library science at the University of Denver and became a librarian.[6] 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. When they returned to Youngstown he attended Rayen High School.[7]

After graduating from

National Research Council fellowship, which he used to study under Gregory Breit at New York University in 1933 and 1934,[12] and then in Copenhagen under Niels Bohr in 1934 and 1935.[13] 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.[9][14]

Early career

The University of North Carolina at Chapel Hill made Wheeler an associate professor in 1937, but he wanted to be able to work more closely with experts in particle physics.[15] 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.[16] He remained a member of its faculty until 1976.[17]

In his 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".[18][19] Wheeler did not pursue this idea, but in the 1940s Werner Heisenberg developed the idea of the S-matrix into an important tool in elementary particle physics.[18]

In 1938 Wheeler joined

Leon Rosenfeld, who informed Wheeler.[16]

Bohr and Wheeler set to work applying the liquid drop model to explain the mechanism of nuclear fission.[23] As the experimental physicists studied fission, they uncovered puzzling results. George Placzek 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 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.[24] They co-wrote two more papers on fission.[25][26] Their first paper appeared in Physical Review on September 1, 1939, the day Germany invaded Poland, starting World War II.[27]

Considering the notion that positrons were electrons traveling backward in time, in 1940 Wheeler conceived his one-electron universe postulate: that there was in fact only one electron, bouncing back and forth in time. His graduate student Richard Feynman found this hard to believe, but the idea that positrons were electrons traveling backward in time intrigued him, and Feynman incorporated the notion of the reversibility of time in his Feynman diagrams.[28]

Nuclear weapons

Manhattan Project

Soon after the Japanese

bombing of Pearl Harbor brought the U.S. into World War II, Wheeler accepted a request from Arthur Compton to join the Manhattan Project's Metallurgical Laboratory at the University of Chicago. He moved there in January 1942,[27] joining Eugene Wigner's group, which was studying nuclear reactor design.[29] He co-wrote a paper with Robert F. Christy on "Chain Reaction of Pure Fissionable Materials in Solution", which was important in the plutonium purification process.[30] It was declassified in December 1955.[31] He gave the neutron moderator its name, replacing Enrico Fermi's term, "slower downer".[32][33]

Loading tubes of the Hanford B Reactor

After the

300 area.[30][36]

Even before the Hanford Site started up the

half life of 6.6 hours, and its daughter product, xenon-135, which has a half life of 9.2 hours. Xenon-135 turned out to have a neutron capture cross-section of well over two million barns. The problem was corrected by adding additional fuel slugs to burn out the poison.[40]

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".[41] 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."[40] Joe left a widow and baby daughter, Mary Jo, who later married physicist James Hartle.[42]

Hydrogen bomb

In August 1945 Wheeler and his family returned to Princeton, where he resumed his academic career.

cosmic rays, and Wheeler became the founder and first director of Princeton's Cosmic Rays Laboratory, which received a grant of $375,000 from the Office of Naval Research in 1948.[49] Wheeler received a Guggenheim Fellowship in 1946,[50] which allowed him to spend the 1949–50 academic year in Paris.[51]

hydrogen bomb
ever tested.

The 1949 detonation of

Los Alamos Laboratory, led by Norris Bradbury.[53][54] Wheeler agreed to go to Los Alamos after a conversation with Bohr.[52] Two of his graduate students from Princeton, Ken Ford and John Toll, joined him there.[55]

At Los Alamos, Wheeler and his family moved into the house on "

Robert Oppenheimer and his family had occupied during the war.[56] In 1950 there was no practical design for a hydrogen bomb. Calculations by Stanisław 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.[57]

In 1951 Wheeler obtained Bradbury's permission to set up a branch office of the Los Alamos laboratory at Princeton, known as

Project Matterhorn, which 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, did nuclear weapons research. Senior scientists remained uninterested and aloof from the project, so he staffed it with young graduate and postdoctoral students.[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, 1952,[59][58] 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]

In January 1953 Wheeler 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.[61][62] This resulted in an official reprimand.[63]

Matterhorn B was discontinued, but Matterhorn S endures as the Princeton Plasma Physics Laboratory.[58]

Later academic career

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 held together in a confined region by the attraction of its own field. He coined the name as a contraction of "gravitational electromagnetic entity".[64] He found that the smallest geon was a toroid the size of the Sun, but millions of times heavier. He later showed that geons are unstable, and would quickly self destruct if they were ever to form.[65]

Geometrodynamics

During the 1950s, Wheeler formulated

gravitation and electromagnetism, to the geometrical properties of a curved space-time. His research on the subject was published in 1957 and 1961.[66][67] Wheeler envisaged the fabric of the universe as a chaotic subatomic realm of quantum fluctuations, which he called "quantum foam".[64][68]

General relativity

University of Moscow, respectively. Wheeler and his students made substantial contributions to the field during the Golden Age of General Relativity.[69]

While working on mathematical extensions to Einstein's general relativity in 1957, Wheeler introduced the concept and word

NASA Goddard Institute of Space Studies (GISS),[72] although the term had been used earlier in the decade.[a] Wheeler said the term was suggested to him during a lecture when a member of the audience was tired of hearing Wheeler say "gravitationally completely collapsed object". Wheeler was also a pioneer in the field of quantum gravity due to his development, with Bryce DeWitt, of the Wheeler–DeWitt equation in 1967.[74] Stephen Hawking later described Wheeler and DeWitt's work as the equation governing the "wave function of the Universe".[75]

Quantum information

Wheeler left Princeton in 1976 at age 65. He was appointed director of the Center for Theoretical Physics at the

Wojciech Zurek
, all former students of Wheeler, wrote:

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 research 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.[77]

quantum physics that he proposed, with the most prominent of them appearing in 1978 and 1984. These experiments seek to discover whether light somehow "senses" the experimental apparatus that it travels through in the double-slit experiment, adjusting its behavior to fit by assuming an appropriate determinate state, or whether it remains in an indeterminate state, neither wave nor particle, and responds to the "questions" the experimental arrangements ask of it in either a wave-consistent manner or a particle-consistent manner.[78]

Teaching

Wheeler's graduate students included

sophomore physics, saying that young minds were the most important. At Princeton he supervised 46 PhDs, more than any other physics professor.[80] Wheeler wrote a supportive review article to help Hugh Everett's work, wrote to and met with Niels Bohr in Copenhagen seeking his approval of Everett's approach, and continued to advocate for Everett even after Bohr's rejection.[81][82]
With Kent Harrison, Kip Thorne, and Masami Wakano, Wheeler wrote Gravitation Theory and Gravitational Collapse (1965). 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.[83] Wheeler and Edwin F. Taylor wrote Spacetime Physics (1966) and Scouting Black Holes (1996).

Alluding to Wheeler's "mass without mass", the festschrift honoring his 60th birthday was titled Magic Without Magic: John Archibald Wheeler: A Collection of Essays in Honor of his Sixtieth Birthday (1972). His writing style could also attract parodies, including one by "John Archibald Wyler" that was affectionately published by a relativity journal.[84][85]

Participatory Anthropic Principle

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.[86][87] He also coined the term "Participatory Anthropic Principle" (PAP), a version of a Strong Anthropic Principle.[88]

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—at 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–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.[89]

In developing the Participatory Anthropic Principle, an

Twenty Questions, called Negative Twenty Questions, to show how the questions we choose to ask about the universe may dictate the answers we get. In this variant, the respondent does not choose or decide upon any particular or definite object beforehand, but only on a pattern of "Yes" or "No" answers. This variant requires the respondent to provide a consistent set of answers to successive questions, so that each answer can be viewed as logically compatible with all the previous ones. In this way, successive questions narrow the options until the questioner settles upon a definite object. Wheeler's theory was that, in an analogous manner, consciousness may play some role in bringing the universe into existence.[90]

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.[91]

Opposition to parapsychology

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 Margaret Mead's request. He called it a pseudoscience,[92] saying he did not oppose earnest research into the questions, but 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.[93] In the question-and-answer period following his presentation "Not consciousness, but the distinction between the probe and the probed, as central to the elemental quantum act of observation", Wheeler incorrectly said that J. B. Rhine had committed fraud as a student, for which he apologized in a subsequent letter to the journal Science.[94] His request was turned down and the Parapsychological Association remained a member of the AAAS.[93]

Personal life

For 72 years, Wheeler was married to Janette Hegner, a teacher and social worker. They became engaged on their third date, but agreed to defer marriage until he returned from Europe. They were married on June 10, 1935, five days after his return.

Arthur Ruark offered Wheeler 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 teach at the Rye Country Day School.[96][16] They had three children.[17]

Wheeler and Hegner were founding members of the Unitarian Church of Princeton, and she initiated the Friends of the Princeton Public Library.[97] In their later years, Hegner accompanied him on sabbaticals in France, Los Alamos, New Mexico, the Netherlands, and Japan.[97] Hegner died in October 2007 at the age of 96.[98][99]

Death and legacy

Wheeler won numerous prizes and awards, including the Golden Plate Award of the

Accademia Nazionale dei Lincei, and the Century Association. He received honorary degrees from 18 different institutions. In 2001, Princeton used a $3 million gift to establish the John Archibald Wheeler/Battelle Professorship in Physics.[17] After his death, the University of Texas named the John A. Wheeler Lecture Hall in his honor.[76]

On April 13, 2008, Wheeler died of pneumonia at the age of 96 in Hightstown, New Jersey.[1]

Bibliography

Notes

  1. ^ American astrophysicist and publisher Hong-Yee Chiu said he remembered a seminar in Princeton University perhaps as early as 1960, when the physicist Robert H. Dicke spoke about gravitationally collapsed objects as "like the Black Hole of Calcutta". According to science writer Marcia Bartusiak, the term had been used in 1963 at an astrophysics conference in Dallas.[73]

References

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  5. ^ Wheeler & Ford 1998, pp. 71–75.
  6. ^ Wheeler & Ford 1998, pp. 78–80.
  7. ^ Leonhart 1939, p. 287.
  8. ^ a b Wheeler & Ford 1998, p. 85.
  9. ^ Wheeler & Ford 1998, p. 97.
  10. ^ a b John Archibald Wheeler at the Mathematics Genealogy Project
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  12. ^ Wheeler & Ford 1998, pp. 123–127.
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  16. ^ a b c d MacPherson, Kitta (April 14, 2008). "Leading physicist John Wheeler dies at age 96". News at Princeton. Archived from the original on April 13, 2016.
  17. ^ a b Mehra & Rechenberg 1982, p. 990.
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  89. ^ Gribbin, Gribbin & Gribbin 2000, pp. 270–271.
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  91. ^ Gardner 1981, pp. 185ff.
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  95. ^ Wheeler & Ford 1998, pp. 144–145.
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  99. American Academy of Achievement
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Sources

External links