John Archibald Wheeler

About John Archibald Wheeler

Who is it?: Physicist
Birth Day: July 09, 1911
Birth Place: Jacksonville, United States
Residence: United States
Alma mater: Johns Hopkins University (Ph.D.)
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 One-electron universe Geon S-matrix Quantum foam Coining the term "neutron moderator" Coining the term "superspace" Coining the term "wormhole" Lorentzian wormhole "It from bit" Participatory anthropic principle
Spouse(s): Janette Hegner
Awards: Albert Einstein Award (1965) Enrico Fermi Award (1968) Franklin Medal (1969) National Medal of Science (1970) Oersted Medal (1983) J. Robert Oppenheimer Memorial Prize (1984) Albert Einstein Medal (1988) Matteucci Medal (1993) Wolf Prize in Physics (1997) Einstein Prize (APS) (2003)
Fields: Physics
Institutions: University of North Carolina Princeton University University of Texas at Austin
Thesis: Theory of the dispersion and absorption of helium (1933)
Doctoral advisor: Karl Herzfeld
Doctoral students: Jacob Bekenstein Claudio Bunster Demetrios Christodoulou Ignazio Ciufolini Hugh Everett Richard Feynman Kenneth W. Ford Robert Geroch John R. Klauder Bahram Mashhoon Charles Misner Milton Plesset Benjamin Schumacher Kip Thorne Jayme Tiomno Bill Unruh Robert Wald Katharine Way Arthur Wightman

John Archibald Wheeler

John Archibald Wheeler was born on July 09, 1911 in Jacksonville, United States, is Physicist. John Archibald Wheeler was a renowned theoretical physicist from America who explained the concept of nuclear fission and fusion. He was instrumental in development of the first atom bomb during World War II and later was involved in the making of the hydrogen bomb. After completing his schooling this scientific genius, associated with the likes of Niels Bohr and Gregory Breit and with the latter he put forth the ‘Breit-Wheeler process’ to convert light into matter. He then began his four decade long association with the Princeton University. It was at Princeton that he developed the concept of S-matrix, which holds good even today. Owing to his expertise in the process of nuclear fission he was inducted into Project Manhattan during WWII. He made significant contribution in the development of nuclear reactor as well as in the purification of Plutonium. After the WWII he resumed his academic responsibilities and was involved in various other research work that included theoretical physics. He spearheaded the revival of theoretical physics and studied the time-space continuum and strived to establish a geometrical basis for phenomenon like gravity. His efforts led to the inception of ‘Geometrodynamics’ and he even studied wormholes and black holes. In fact he was the one to coin the term black hole. Read on to know more about his life and works
John Archibald Wheeler is a member of Scientists

Does John Archibald Wheeler Dead or Alive?

As per our current Database, John Archibald Wheeler has been died on April 13, 2008(2008-04-13) (aged 96)\nHightstown, New Jersey, United States.

🎂 John Archibald Wheeler - Age, Bio, Faces and Birthday

When John Archibald Wheeler die, John Archibald Wheeler was 96 years old.

Popular As John Archibald Wheeler
Occupation Scientists
Age 96 years old
Zodiac Sign Leo
Born July 09, 1911 (Jacksonville, United States)
Birthday July 09
Town/City Jacksonville, United States
Nationality United States

🌙 Zodiac

John Archibald Wheeler’s zodiac sign is Leo. According to astrologers, people born under the sign of Leo are natural born leaders. They are dramatic, creative, self-confident, dominant and extremely difficult to resist, able to achieve anything they want to in any area of life they commit to. There is a specific strength to a Leo and their "king of the jungle" status. Leo often has many friends for they are generous and loyal. Self-confident and attractive, this is a Sun sign capable of uniting different groups of people and leading them as one towards a shared cause, and their healthy sense of humor makes collaboration with other people even easier.

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Famous Quotes:

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.



Wheeler was born in Jacksonville, Florida on July 9, 1911 to librarians Joseph Lewis Wheeler and Mabel Archibald (Archie) Wheeler. He was the oldest of four children, having two younger brothers, Joseph and Robert, and a younger sister, Mary. Joseph earned a 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. 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.


After graduating from the Baltimore City College high school in 1926, Wheeler entered Johns Hopkins University with a scholarship from the state of Maryland. He published his first scientific paper in 1930, as part of a summer job at the National Bureau of Standards. 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". He received a National Research Council fellowship, which he used to study under Gregory Breit at New York University in 1933 and 1934, and then in Copenhagen under Niels Bohr in 1934 and 1935. 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.


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 after he returned from Europe. They were married on June 10, 1935, five days after his return. Jobs were hard to come by during the Great Depression, but 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. They had three children: Letitia, James English and Alison Wheeler.


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." Werner Heisenberg subsequently 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.


Wheeler did not develop the S-matrix, but joined Edward Teller in examining Bohr's liquid drop model of the atomic nucleus. 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. The news of Lise Meitner and Otto Frisch's discovery of fission was brought to America by Bohr in 1939. Bohr told Leon Rosenfeld, who informed Wheeler.


Bohr and Wheeler set to work applying the liquid drop model to explain the mechanism of nuclear fission. 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 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. They co-wrote two more papers on fission. Their first paper appeared in Physical Review on September 1, 1939, the day Germany invaded Poland, starting World War II in Europe.


Considering the notion that positrons were electrons that were traveling backwards in time, he came up in 1940 with 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 backwards in time intrigued him and Feynman incorporated the notion of the reversibility of time into his Feynman diagrams.


Soon after the Japanese bombing of Pearl Harbor brought the United States 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, joining Eugene Wigner's group, which was studying nuclear reactor design. 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. It would not be declassified until December 1955. He gave the neutron moderator its name, replacing the term "slower downer" used by Enrico Fermi.


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. Wheeler became part of the DuPont design staff. He worked closely with its Engineers, commuting between Chicago and Wilmington, Delaware, where DuPont had its headquarters. He moved his family to Wilmington in March 1943. DuPont's task was not just to build nuclear reactors, but an entire plutonium production complex at the Hanford Site in Washington. 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.


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". 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." Joe left a widow and baby daughter, Mary Jo, who later married Physicist James Hartle.


In August 1945 Wheeler and his family returned to Princeton, where he resumed his academic career. Working with Feynman, he explored the possibility of physics with particles, but not fields, and carried out theoretical studies of the muon with Jayme Tiomno, resulting in a series of papers on the topic, including a 1949 paper in which Tiomno and Wheeler introduced the "Tiomno Triangle", which related different forms of radioactive decay. He also suggested the use of muons as a nuclear probe. This paper, written and privately circulated in 1949 but not published until 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. He received a Guggenheim Fellowship in 1946, which allowed him to spend the 1949–50 academic year in Paris.


The 1949 detonation of Joe-1 by the Soviet Union prompted an all-out effort by the United States, led by Teller, to develop the more powerful hydrogen bomb in response. 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. Those 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. Wheeler agreed to go to Los Alamos after a conversation with Bohr. Two of his graduate students from Princeton, Ken Ford and John Toll, joined him there.


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. His research on the subject was published in 1957 and 1961. Wheeler envisaged the fabric of the universe as a chaotic sub-atomic realm of quantum fluctuations, which he called "quantum foam".


In 1951 Wheeler obtained permission from Bradbury 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, engaged in nuclear weapons research. Senior Scientists remained uninterested and aloof from the project, so he staffed it with young graduate and post-doctoral students. 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 an official reprimand. 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, 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. Matterhorn B was discontinued, but Matterhorn S endures as the Princeton Plasma Physics Laboratory.


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 that 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." He found that the smallest geon was a toroid the size of the Sun, but millions of times heavier.


While working on mathematical extensions to Einstein's Theory of General Relativity in 1957, Wheeler introduced the concept and word wormhole to describe hypothetical "tunnels" in space-time. Bohr asked if they were stable and further research by Wheeler determined that they are not. 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).


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. Wheeler gave a high priority to teaching, and continued to teach freshman and sophomore physics, saying that the young minds were the most important. 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. Wheeler teamed up with Edwin F. Taylor to write Spacetime Physics (1966) and Scouting Black Holes (1996). At Princeton he supervised 46 PhDs, more than any other professor in the Princeton physics department.


Wheeler won numerous prizes and awards, including the Enrico Fermi Award in 1968, the Franklin Medal in 1969, the Einstein Prize in 1969, the National Medal of Science in 1971, 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. 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. In 2001, Princeton used a $3 million gift to establish the John Archibald Wheeler/Battelle Professorship in Physics. After his death, the University of Texas named the John A. Wheeler Lecture Hall in his honor.


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.


Wheeler left Princeton University in 1976 at the age of 65. He was appointed as the Director of the Center for Theoretical Physics at the University of Texas at Austin in 1976 and remained in the position until 1986, when he retired and became a professor emeritus. Misner, Thorne and Wojciech Zurek, all former students of Wheeler, wrote that:


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".


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, 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. 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 stated that J. B. Rhine had committed fraud as a student, for which he apologized in a subsequent letter to the journal Science. His request was turned down and the Parapsychological Association remained a member of the AAAS.


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


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


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. Stephen Hawking later described Wheeler and DeWitt's work as the equation governing the "wave function of the Universe".

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