Hans Bethe

Hans Albrecht Bethe (German: [ˈhans ˈalbʁɛçt ˈbeːtə]; July 2, 1906 – March 6, 2005) was a German-American nuclear physicist who made important contributions to astrophysics, quantum electrodynamics and solid-state physics, and won the 1967 Nobel Prize in Physics for his work on the theory of stellar nucleosynthesis.[1][2]

For most of his career, Bethe was a professor at Cornell University.[3] During World War II, he was head of the Theoretical Division at the secret Los Alamos laboratory which developed the first atomic bombs. There he played a key role in calculating the critical mass of the weapons and developing the theory behind the implosion method used in both the Trinity test and the "Fat Man" weapon dropped on Nagasaki in August 1945.

After the war, Bethe also played an important role in the development of the hydrogen bomb, though he had originally joined the project with the hope of proving it could not be made. Bethe later campaigned with Albert Einstein and the Emergency Committee of Atomic Scientists against nuclear testing and the nuclear arms race. He helped persuade the Kennedy and Nixon administrations to sign, respectively, the 1963 Partial Nuclear Test Ban Treaty and 1972 Anti-Ballistic Missile Treaty (SALT I).

His scientific research never ceased and he was publishing papers well into his nineties, making him one of the few scientists to have published at least one major paper in his field during every decade of his career – which, in Bethe's case, spanned nearly seventy years. Freeman Dyson, once one of his students, called him the "supreme problem-solver of the 20th century".[4]

Hans Bethe
Hans Bethe
Born
Hans Albrecht Bethe

July 2, 1906
DiedMarch 6, 2005 (aged 98)
Ithaca, New York, United States
ResidenceGermany
United States
NationalityGerman
American
Alma materUniversity of Frankfurt
University of Munich
Known for
Spouse(s)
Rose Ewald (married in 1939; two children)
Awards
Scientific career
FieldsNuclear physics
Institutions
Doctoral advisorArnold Sommerfeld
Doctoral students
Other notable studentsFreeman Dyson
Signature
Hans Bethe (signature)

Early years

Bethe was born in Strasbourg, which was then part of Germany, on July 2, 1906, the only child of Anna (née Kuhn) and Albrecht Bethe, a privatdozent of physiology at the University of Strasbourg.[5] Although his mother, the daughter of a professor at the University of Strasbourg, was Jewish,[6] he was raised a Protestant like his father.[7] Despite having a religious background,[8] he was not religious in later life, and described himself as an atheist.[9]

Hans Bethe, aged 12
Hans Bethe, aged 12, with his parents

His father accepted a position as professor and director of the Institute of Physiology at the University of Kiel in 1912, and the family moved into the director's apartment at the Institute. He was initially schooled privately by a professional teacher as part of a group of eight girls and boys.[10] The family moved again in 1915 when his father became the head of the new Institute of Physiology at the University of Frankfurt am Main.[7]

Bethe attended the Goethe-Gymnasium in Frankfurt, Germany. His education was interrupted in 1916, when he contracted tuberculosis, and he was sent to Bad Kreuznach to recuperate. By 1917, he had recovered sufficiently to attend the local realschule, and the following year he was sent to the Odenwaldschule, a private, coeducational boarding school.[11] He attended the Goethe-Gymnasium again for his final three years of secondary schooling, from 1922 to 1924.[12]

Having passed his abitur, Bethe entered the University of Frankfurt in 1924. He decided to major in chemistry. The instruction in physics was poor, and while there were distinguished mathematicians in Frankfurt like Carl Ludwig Siegel and Otto Szász, Bethe disliked their approaches, which presented mathematics without reference to the other sciences.[13] Bethe found that he was a poor experimentalist who destroyed his lab coat by spilling sulfuric acid on it, but he found the advanced physics taught by the associate professor, Walter Gerlach, more interesting.[13][14] Gerlach left in 1925, and was replaced by Karl Meissner, who advised Bethe that he should go to a university with a better school of theoretical physics, specifically the University of Munich, where he could study under Arnold Sommerfeld.[15][16]

Bethe entered the University of Munich in April 1926, where Sommerfeld took him on as a student on Meissner's recommendation.[17] Sommerfeld taught an advanced course on differential equations in physics, which Bethe enjoyed. Because he was such a renowned scholar, Sommerfeld frequently received advance copies of scientific papers, which he put up for discussion at weekly evening seminars. When Bethe arrived, Sommerfeld had just received Erwin Schrödinger's papers on wave mechanics.[18]

For his PhD thesis, Sommerfeld suggested that Bethe examine electron diffraction in crystals. As a starting point, Sommerfeld suggested Paul Ewald's 1914 paper on X-ray diffraction in crystals. Bethe later recalled that he became too ambitious, and, in pursuit of greater accuracy, his calculations became unnecessarily complicated.[19] When he met Wolfgang Pauli for the first time, Pauli told him: "After Sommerfeld's tales about you, I had expected much better from you than your thesis."[20] "I guess from Pauli," Bethe later recalled, "that was a compliment."[20]

Early work

After Bethe received his doctorate, Erwin Madelung offered him an assistantship in Frankfurt, and in September 1928 Bethe moved in with his father, who had recently divorced his mother. His father met Vera Congehl earlier that year, and married her in 1929. They had two children, Doris, born in 1933, and Klaus, born in 1934.[21] Bethe did not find the work in Frankfurt very stimulating, and in 1929 he accepted an offer from Ewald at the Technische Hochschule in Stuttgart. While there, he wrote what he considered to be his greatest paper,[22] Zur Theorie des Durchgangs schneller Korpuskularstrahlen durch Materie ("The Theory of the Passage of Fast Corpuscular Rays Through Matter").[23] Starting from Max Born's interpretation of the Schrödinger equation, Bethe produced a simplified formula for collision problems using a Fourier transform, which is known today as the Bethe formula. He submitted this paper for his habilitation in 1930.[22][24][25]

Sommerfeld recommended Bethe for a Rockefeller Foundation Travelling Scholarship in 1929. This provided $150 a month (about $2,000 in 2018 dollars[A]) to study abroad. In 1930, Bethe chose to do postdoctoral work at the Cavendish Laboratory at the University of Cambridge in England, where he worked under the supervision of Ralph Fowler.[26] At the request of Patrick Blackett, who was working with cloud chambers, Bethe created a relativistic version of the Bethe formula.[27] Bethe was also known for his sense of humor, and with Guido Beck and Wolfgang Riezler, two other postdoctoral research fellows, created a hoax paper On the Quantum Theory of the Temperature of Absolute Zero where he calculated the fine structure constant from the absolute zero temperature in Celsius units.[28] The paper poked fun at a certain class of papers in theoretical physics of the day, which were purely speculative and based on spurious numerical arguments such as Arthur Eddington's attempts to explain the value of the fine structure constant from fundamental quantities in an earlier paper. They were forced to issue an apology.[29]

For the second half of his scholarship, Bethe chose to go to Enrico Fermi's laboratory in Rome in February 1931. He was greatly impressed by Fermi and regretted that he had not gone to Rome first.[30] Bethe developed the Bethe ansatz, a method for finding the exact solutions for the eigenvalues and eigenvectors of certain one-dimensional quantum many-body models.[31] He was influenced by Fermi's simplicity and Sommerfeld's rigor in approaching problems, and these qualities influenced his own later research.[32]

The Rockefeller Foundation offered an extension of Bethe's fellowship, allowing him to return to Italy in 1932.[33] In the meantime, Bethe worked for Sommerfeld in Munich as a privatdozent. Since Bethe was fluent in English, Sommerfeld had Bethe supervise all his English-speaking postdoctoral fellows, including Lloyd P. Smith from Cornell University.[34] Bethe accepted a request from Karl Scheel to write an article for the Handbuch der Physik on the quantum mechanics of hydrogen and helium. Reviewing the article decades later, Robert Bacher and Victor Weisskopf noted that it was unusual in the depth and breadth of its treatment of the subject, yet required very little updating for the 1959 edition. Bethe was then asked by Sommerfeld to help him with the handbuch article on electrons in metals. The article covered the basis of what is now called solid state physics. Bethe took a very new field and provided a clear, coherent and complete coverage of it.[33] His work on the handbuch articles occupied most of his time in Rome, but he also co-wrote a paper with Fermi on another new field, quantum electrodynamics, describing the relativistic interactions of charged particles.[35]

In 1932, Bethe accepted an appointment as an assistant professor at the University of Tübingen, where Hans Geiger was the professor of experimental physics.[36][37] One of the first laws passed by the new National Socialist government was the Law for the Restoration of the Professional Civil Service. Due to his Jewish background, Bethe was dismissed from his job at the University, which was a government post. Geiger refused to help, but Sommerfeld immediately gave Bethe back his fellowship at Munich. Sommerfeld spent much of the summer term of 1933 finding places for Jewish students and colleagues.[38]

Bethe left Germany in 1933, moving to England after receiving an offer for a position as lecturer at the University of Manchester for a year through Sommerfeld's connection to William Lawrence Bragg.[38] He moved in with his friend Rudolf Peierls and Peierls' wife Genia. Peierls was a fellow Jewish German physicist who had also been barred from academic positions in Germany. This meant that Bethe had someone to speak to in German, and did not have to eat English food.[39] Their relationship was professional as well as personal. Peierls aroused Bethe's interest in nuclear physics.[40] After James Chadwick and Maurice Goldhaber discovered the photodisintegration of deuterium,[41] Chadwick challenged Bethe and Peierls to come up with a theoretical explanation of this phenomenon. This they did on the four-hour train ride from Cambridge back to Manchester.[42] Bethe would investigate further in the years ahead.[40]

In 1933, the physics department at Cornell was looking for a new theoretical physicist, and Lloyd Smith strongly recommended Bethe. This was supported by Bragg, who was visiting Cornell at the time. In August 1934, Cornell offered Bethe a position as an acting assistant professor. Bethe had already accepted a fellowship for a year to work with Nevill Mott at the University of Bristol for a semester, but Cornell agreed to let him start in the spring of 1935.[43] Before leaving for the United States, he visited the Niels Bohr Institute in Copenhagen in September 1934, where he proposed to Hilde Levi, who accepted. However, the match was opposed by Bethe's mother, who did not want him marrying a Jewish girl, despite being Jewish herself, and Bethe broke off their engagement a few days before their wedding date in December.[44] Niels Bohr and James Franck were so shocked by Bethe's behavior that he was not invited to the Institute again until after World War II.[45]

United States

Bethe arrived in the United States in February 1935, and joined the faculty at Cornell University on a salary of $3,000.[46] Bethe's appointment was part of a deliberate effort on the part of the new head of its physics department, Roswell Clifton Gibbs, to move into nuclear physics.[47] Gibbs had hired Stanley Livingston, who had worked with Ernest Lawrence, to build a cyclotron at Cornell.[47] To complete the team, Cornell needed an experimentalist, and, on the advice of Bethe and Livingston, recruited Robert Bacher. Bethe received requests to visit Columbia University from Isidor Isaac Rabi, Princeton University from Edward Condon, University of Rochester from Lee DuBridge, Purdue University from Karl Lark-Horovitz, the University of Illinois at Urbana–Champaign from Francis Wheeler Loomis, and Harvard University from John Hasbrouck Van Vleck. Gibbs moved to prevent Bethe from being poached by having him appointed as a regular assistant professor in 1936, with an assurance that promotion to professor would soon follow.[48]

Together with Bacher and Livingston, Bethe published a series of three articles,[49][50][51] which summarized most of what was known on the subject of nuclear physics until that time, an account that became informally known as "Bethe's Bible", and remained the standard work on the subject for many years. In this account, he also continued where others left off, filling in gaps in the older literature.[52] Loomis offered Bethe a full professorship at the University of Illinois at Urbana–Champaign, but Cornell matched the offer, and the salary of $6,000.[53] He wrote to his mother:

I am about the leading theoretician in America. That does not mean the best. Wigner is certainly better and Oppenheimer and Teller probably just as good. But I do more and talk more and that counts too.[54]

FusionintheSun
Illustration of the proton–proton chain reaction sequence
CNO Cycle
Overview of the CNO-I cycle. The helium nucleus is released at the top-left step.

On March 17, 1938, Bethe attended the Carnegie Institute and George Washington University's fourth annual Washington Conference of Theoretical Physics. There were only 34 invited attendees, but they included Gregory Breit, Subrahmanyan Chandrasekhar, George Gamow, Donald Menzel, John von Neumann, Bengt Strömgren, Edward Teller and Merle Tuve. Bethe initially declined the invitation to attend, because the conference's topic, stellar energy generation, did not interest him, but Teller persuaded him to come. At the conference, Strömgren detailed what was known about the temperature, density and chemical composition of the Sun, and challenged the physicists to come up with an explanation. Gamow and Carl Friedrich von Weizsäcker had proposed in a 1937 paper that the Sun's energy was the result of a proton–proton chain reaction:[55][56]


p
 

p
→  2
1
D
 

e+
 

ν
e

But this did not account for the observation of elements heavier than helium. By the end of the conference, Bethe, working in collaboration with Charles Critchfield, had come up with a series of subsequent nuclear reactions that explained how the Sun shines:[57]

2
1
D
 

p
 
→  3
2
He
 

γ
3
2
He
 
3
2
He
 
→  4
2
He
 

p
3
2
He
 
4
2
He
 
→  7
4
Be
 

γ
7
4
Be
 

e
 
→  7
3
Li
 

ν
e
7
3
Li
 

p
 
→  4
2
He

That this did not explain the processes in heavier stars was not overlooked. At the time there were doubts about whether the proton–proton cycle described the processes in the Sun, but more recent measurements of the Sun's core temperature and luminosity show that it does.[55] When he returned to Cornell, Bethe studied the relevant nuclear reactions and reaction cross sections, leading to his discovery of the carbon-nitrogen-oxygen cycle (CNO cycle):[58]

12
6
C
 

p
 
→  13
7
N
 

γ
13
7
N
 
    →  13
6
C
 

e+
 

ν
e
13
6
C
 

p
 
→  14
7
N
 

γ
14
7
N
 

p
 
→  15
8
O
 

γ
15
8
O
 
    →  15
7
N
 

e+
 

ν
e
15
7
N
 

p
 
→  12
6
C
 
4
2
He

The two papers, one on the proton–proton cycle, co-authored with Critchfield, and the other on the carbon-oxygen-nitrogen (CNO) cycle, were sent to the Physical Review for publication.[59] After Kristallnacht, Bethe's mother had become afraid to remain in Germany. Taking advantage of her Strasbourg origin, she was able to emigrate to the United States in June 1939 on the French quota, rather than the German one, which was full.[60] Bethe's graduate student Robert Marshak noted that the New York Academy of Sciences was offering a $500 prize for the best unpublished paper on the topic of solar and stellar energy. So Bethe, in need of $250 to release his mother's furniture, withdrew the CNO cycle paper and sent it in to the New York Academy of Sciences. It won the prize, and Bethe gave Marshak $50 finder's fee and used $250 to release his mother's furniture. The paper was subsequently published in the Physical Review in March. It was a breakthrough in the understanding of the stars, and would win Bethe the Nobel Prize in Physics in 1967.[61][59] In 2002, at age 96, Bethe sent a handwritten note to John N. Bahcall congratulating him on the use of solar neutrino observations to show that the CNO cycle accounts for about 7% of the Sun's energy; the neutrino observations had started with Raymond Davis Jr., whose experiment was based on Bahcall's calculations and encouragement, and led to Davis's receiving a share of the 2002 Nobel Prize.[62]

Bethe married Rose Ewald, the daughter of Paul Ewald, on September 13, 1939, in a simple civil ceremony.[63] They had two children, Henry and Monica.[64] (Henry was a contract bridge expert and former husband of Kitty Munson Cooper.)[65] He became a naturalized citizen of the United States in March 1941.[66] Writing to Sommerfeld in 1947, Bethe confided that "I am much more at home in America than I ever was in Germany. As if I was born in Germany only by mistake, and only came to my true homeland at 28."[67]

Manhattan Project

Hans Bethe ID badge
Bethe's Los Alamos Laboratory ID badge

When the Second World War began, Bethe wanted to contribute to the war effort,[68] but was unable to work on classified projects until he became a citizen. Following the advice of the Caltech aerodynamicist Theodore von Kármán, Bethe collaborated with his friend Teller on a theory of shock waves which are generated by the passage of a projectile through a gas. Bethe considered it one of their most influential papers. He also worked on a theory of armor penetration, which was immediately classified by the Army, making it inaccessible to Bethe, who was not an American citizen at the time.[69]

After receiving security clearance in December 1941, Bethe joined the MIT Radiation Laboratory, where he invented the Bethe-hole directional coupler, which is used in microwave waveguides such as those used in radar sets.[70] In Chicago in June 1942, and then at the University of California, Berkeley, in July, he participated in a series of meetings at the invitation of Robert Oppenheimer, which discussed the first designs for the atomic bomb. They went over the preliminary calculations by Robert Serber, Stan Frankel, and others, and discussed the possibilities of using uranium-235 and plutonium. Teller then raised the prospect of a thermonuclear device, Teller's "Super" bomb. At one point Teller asked if the nitrogen in the atmosphere could be set alight. It fell to Bethe and Emil Konopinski to perform the calculations to prove that this could not occur.[71] "The fission bomb had to be done," he later recalled, "because the Germans were presumably doing it."[72]

When Oppenheimer was put in charge of forming a secret weapons design laboratory, Los Alamos, he appointed Bethe director of the T (Theoretical) Division, the laboratory's smallest but most prestigious division. This move irked the equally qualified but more difficult to manage Teller and Felix Bloch, who had coveted the job.[73][74] A series of disagreements between Bethe and Teller between February and June 1944 over the relative priority of Super research led to Teller's group being removed from T Division and placed directly under Oppenheimer. In September it became part of Fermi's new F Division.[75]

Bethe's work at Los Alamos included calculating the critical mass and efficiency of uranium-235 and the multiplication of nuclear fission in an exploding atomic bomb. Along with Richard Feynman, he developed a formula for calculating the bomb's explosive yield.[76] After August 1944, when the laboratory was reorganized and reoriented to solve the problem of the implosion of the plutonium bomb, Bethe spent much of his time studying the hydrodynamic aspects of implosion, a job which he continued into 1944.[77] In 1945, he worked on the neutron initiator, and later on radiation propagation from an exploding atomic bomb.[78] The Trinity nuclear test validated the accuracy of T Division's results.[79] When it was detonated in the New Mexico desert on July 16, 1945, Bethe's immediate concern was for its efficient operation, and not its moral implications. He is reported to have commented: "I am not a philosopher."[80]

Hydrogen bomb

After the war, Bethe argued that a crash project for the hydrogen bomb should not be attempted, though after President Harry Truman announced the beginning of such a project, and the outbreak of the Korean War, Bethe signed up and played a key role in the weapon's development. Though he would see the project through to its end, Bethe hoped that it would be impossible to create the hydrogen bomb.[81] He would later remark in 1968 on the apparent contradiction in his stance, having first opposed the development of the weapon and later helping to create it:

Just a few months before, the Korean war had broken out, and for the first time I saw direct confrontation with the communists. It was too disturbing. The cold war looked as if it were about to get hot. I knew then I had to reverse my earlier position. If I did not work on the bomb, somebody else would — and I had thought if I were around Los Alamos I might still be a force for disarmament. So I agreed to join in developing the H-bomb. It seemed quite logical. But sometimes I wish I were a more consistent idealist.[82]

As for his own role in the project, and its relation to the dispute over who was responsible for the design, Bethe later said that:

After the H-bomb was made, reporters started to call Teller the father of the H-bomb. For the sake of history, I think it is more precise to say that Ulam is the father, because he provided the seed, and Teller is the mother, because he remained with the child. As for me, I guess I am the midwife.[82]

In 1954, Bethe testified on behalf of J. Robert Oppenheimer during the Oppenheimer security hearing. Specifically, Bethe argued that Oppenheimer's stances against developing the hydrogen bomb in the late 1940s had not hindered its actual development, a topic which was seen as a key motivating factor behind the hearing. Bethe contended that the developments which led to the successful Teller–Ulam design were a matter of serendipity and not a question of manpower or logical development of previously existing ideas. During the hearing, Bethe and his wife also tried hard to convince Edward Teller against testifying. However, Teller did not agree, and his testimony played a major role in the revocation of Oppenheimer's security clearance. While Bethe and Teller had been on very good terms during the prewar years, the conflict between them during the Manhattan Project, and especially during the Oppenheimer episode, permanently marred their relationship.[83]

Later work

Lamb shift

Bethe hans
Hans Bethe lecturing at Dalhousie University, 1978.

After the war ended, Bethe returned to Cornell. In June 1947, he participated in the Shelter Island Conference. Sponsored by the National Academy of Sciences and held at the Ram's Head Inn on Shelter Island, New York, the conference on the "Foundations of Quantum Mechanics" was the first major physics conference held since the war. It was a chance for American physicists to come together, pick up where they had left off before the war, and establish the direction of post-war research.[84][85]

A major talking point at the conference was the discovery by Willis Lamb and his graduate student Robert Retherford shortly before the conference began that one of the two possible quantum states of hydrogen atoms had slightly more energy than predicted by the Paul Dirac's theory; this became known as the Lamb shift. Oppenheimer and Weisskopf suggested that this was a result of quantum fluctuations of the electromagnetic field. Pre-war quantum electrodynamics (QED) gave absurd, infinite values for this; but the Lamb shift showed that it was both real and finite. Hans Kramers proposed renormalization as a solution, but no one knew how to do the calculation.[86][84]

Bethe managed to work it out on the train from New York to Schenectady. He arrived at a value of 1040 MHz, extremely close to that obtained experimentally by Lamb and Retherford. He did so by realising that it was a non-relativistic process, which greatly simplified the calculations. His paper, published in the Physical Review in August 1947 was only two pages long and contained just 12 mathematical equations, but was enormously influential. Hitherto, it had been assumed that the infinities meant that QED was fundamentally flawed, and that a new, radical theory was required. Bethe demonstrated that this was not necessary.[87] One of Bethe's most famous papers is one he never wrote: the 1948 Alpher–Bethe–Gamow paper.[88] George Gamow added Bethe's name (in absentia) without consulting him, knowing that Bethe would not mind, and against Ralph Alpher's wishes. This was apparently a reflection of Gamow's sense of humor, wanting to have a paper title that would sound like the first three letters of the Greek alphabet. As one of the Physical Review's reviewers, Bethe saw the manuscript and struck out the words "in absentia".[89]

Astrophysics

Bethe believed that the atomic nucleus was like a quantum liquid drop. He investigated the nuclear matter problem by considering the work done by Keith Brueckner on perturbation theory. Working with Jeffrey Goldstone, he produced a solution for the case where there was an infinite hard-core potential. Then, working with Baird Brandow and Albert Petschek, he came up with an approximation that converted the scattering equation into an easily solved differential equation. This then led him to the Bethe-Faddeev equation, a generalisation of Ludvig Faddeev's approach to three-body scattering. He then used these techniques to examine the neutron stars, which have densities similar to those of nuclei.[90]

Bethe continued to do research on supernovae, neutron stars, black holes, and other problems in theoretical astrophysics into his late nineties. In doing this, he collaborated with Gerald E. Brown of Stony Brook University. In 1978, Brown proposed that they collaborate on supernovae. These were reasonably well understood by this time, but the calculations were still a problem. Using techniques honed from decades of working with nuclear physics, and some experience with calculations involving nuclear explosions, Bethe tackled the problems involved in stellar gravitational collapse, and the way in which various factors affected a supernova explosion. Once again, he was able to reduce the problem to a set of differential equations, and solve them.[91][92]

At age 85, Bethe wrote an important article about the solar neutrino problem, in which he helped establish the conversion mechanism for electron neutrinos into muon neutrinos proposed by Stanislav Mikheyev, Alexei Smirnov and Lincoln Wolfenstein to explain a vexing discrepancy between theory and experiment. Bethe argued that physics beyond the Standard Model was required to understand the solar neutrino problem, because it assumed that neutrinos have no mass, and therefore cannot metamorphosize into each other; whereas the MSW effect required this to occur. Bethe hoped that corroborating evidence would be found by the Sudbury Neutrino Observatory (SNO) in Ontario, Canada, by his 90th birthday, but he did not get the call from SNO until June 2001, when he was nearly 95.[93][94]

In 1996, Kip Thorne approached Bethe and Brown about LIGO, the Laser Interferometer Gravitational-Wave Observatory, designed to detect the gravitational waves from merging neutron stars and black holes. Since Bethe and Brown were good at calculating things that could not be seen, could they look at the mergers? The 90-year-old Bethe quickly became enthused, and soon began the required calculations. The result was a 1998 paper on the "Evolution of Binary Compact Objects Which Merge", which Brown regarded as the best that the two produced together.[95][96]

Political stances

Hans Albrecht Bethe (1906-2005)
Bethe being interviewed by journalists

In 1968, Bethe, along with IBM physicist Richard Garwin, published an article criticising in detail the anti-ICBM defense system proposed by the Department of Defense. The two physicists described in the article that nearly any measure taken by the US would be easily thwarted with the deployment of relatively simple decoys.[97] Bethe was one of the primary voices in the scientific community behind the signing of the 1963 Partial Test Ban Treaty prohibiting further atmospheric testing of nuclear weapons.[98]

During the 1980s and 1990s, Bethe campaigned for the peaceful use of nuclear energy. After the Chernobyl disaster, Bethe was part of a committee of experts that analysed the incident. They concluded that the reactor suffered from a fundamentally faulty design and human error also had significantly contributed to the accident. "My colleagues and I established," he explained "that the Chernobyl disaster tells us about the deficiencies of the Soviet political and administrative system rather than about problems with nuclear power."[99] Throughout his life Bethe remained a strong advocate for electricity from nuclear energy, which he described in 1977 as "a necessity, not merely an option."[100]

In the 1980s he and other physicists opposed the Strategic Defense Initiative missile system conceived by the Ronald Reagan administration.[101] In 1995, at the age of 88, Bethe wrote an open letter calling on all scientists to "cease and desist" from working on any aspect of nuclear weapons development and manufacture.[102] In 2004, he joined 47 other Nobel laureates in signing a letter endorsing John Kerry for President of the United States as someone who would "restore science to its appropriate place in government".[103]

Historian Gregg Herken wrote:

When Oppenheimer died, Oppie's long-time friend, Hans Bethe, assumed the mantle of the scientist of conscience in this country. Like Jefferson and Adams, Teller and Bethe would live on into the new century which they and their colleagues had done so much to shape.[104]

Personal life

Bethe's hobbies included a passion for stamp-collecting.[105] He loved the outdoors, and was an enthusiastic hiker all his life, exploring the Alps and the Rockies.[106] He died in his home in Ithaca, New York on March 6, 2005 [107] of congestive heart failure.[72] He was survived by his wife Rose and two children.[108] At the time of his death, he was the John Wendell Anderson Professor of Physics, Emeritus at Cornell University.[109]

Honors and awards

Bethe received numerous honors and awards in his lifetime and afterwards. He became a Fellow of the American Academy of Arts and Sciences in 1947,[110] and that year was received the National Academy of Sciences's Henry Draper Medal.[111] He was awarded the Max Planck Medal in 1955, the Franklin Medal in 1959, the Royal Astronomical Society's Eddington Medal and the United States Atomic Energy Commission's Enrico Fermi Award in 1961,[112] the Rumford Prize in 1963,[113] the Nobel Prize in Physics in 1967,[64] the National Medal of Science in 1975,[114] Oersted Medal in 1993,[115] the Bruce Medal in 2001,[116] and the Benjamin Franklin Medal for Distinguished Achievement in the Sciences by the American Philosophical Society posthumously in 2005.[117]

Bethe was elected Foreign Member of the Royal Society (ForMemRS) in 1957,[1] and he gave the 1993 Bakerian Lecture at the Royal Society on the Mechanism of Supernovae.[118] In 1978 he was elected a Member of the German Academy of Sciences Leopoldina.[119]

Cornell named the third of five new residential colleges, each of which is named after a distinguished former member of the Cornell faculty, Hans Bethe House after him,[120] as was the Hans Bethe Center, 322 4th St. NE, Washington, DC, home to the Council for a Livable World, where Bethe was a longtime board member,[121] and the Bethe Center for Theoretical Physics at University of Bonn in Germany.[122] He also has an asteroid, 30828 Bethe, that was discovered in 1990 named after him,[123] as was the American Physical Society's Hans Bethe Prize.[124]

Selected publications

Notes

  1. ^ Federal Reserve Bank of Minneapolis Community Development Project. "Consumer Price Index (estimate) 1800–". Federal Reserve Bank of Minneapolis. Retrieved January 2, 2019.

Citations

  1. ^ a b c Lee, S.; Brown, G. E. (2007). "Hans Albrecht Bethe. 2 July 1906 -- 6 March 2005: Elected ForMemRS 1957". Biographical Memoirs of Fellows of the Royal Society. 53: 1. doi:10.1098/rsbm.2007.0018.
  2. ^ Horgan, John (1992). "Illuminator of the Stars". Scientific American. 267 (4): 32. Bibcode:1992SciAm.267d..32H. doi:10.1038/scientificamerican1092-32.
  3. ^ Available at www.JamesKeckCollectedWorks.org [1] are the class notes taken by one of his students at Cornell from the graduate courses on Nuclear Physics and on Applications of Quantum Mechanics he taught in the spring of 1947.
  4. ^ Wark, David (11 January 2007). "The Supreme Problem Solver". Nature. 445 (7124): 149. Bibcode:2007Natur.445..149W. doi:10.1038/445149a.
  5. ^ Bernstein 1980, p. 7.
  6. ^ Bernstein 1980, p. 8.
  7. ^ a b Schweber 2012, pp. 32–34.
  8. ^ "Interview with Hans Bethe by Charles Weiner at Cornell University". American Institute of Physics. November 17, 1967. Retrieved 25 April 2012. When asked by Charles Weiner if there was religion in his home, Bethe replied: "No. My father was, I think, slightly religious. I was taught to pray in the evening before going to bed, and I attended the Protestant religious instruction, which was given in the schools in Germany. I was also confirmed, and the instruction which I got in this connection got religion out of my system completely. It was never very strong before, and the confirmation had the consequence that I just didn't believe."
  9. ^ Brian 2001, p. 117.
  10. ^ Schweber 2012, pp. 30–31.
  11. ^ Schweber 2012, pp. 36–40.
  12. ^ Schweber 2012, p. 45.
  13. ^ a b Bernstein 1980, pp. 11–12.
  14. ^ Schweber 2012, pp. 70–73.
  15. ^ Bernstein 1980, p. 13.
  16. ^ Schweber 2012, p. 93.
  17. ^ Schweber 2012, pp. 118–119.
  18. ^ Bernstein 1980, pp. 15–16.
  19. ^ Bernstein 1980, pp. 20–21.
  20. ^ a b Schweber 2012, p. 142.
  21. ^ Schweber 2012, pp. 156–157.
  22. ^ a b Bernstein 1980, pp. 25–27.
  23. ^ Bethe, Hans (1930). "Zur Theorie des Durchgangs schneller Korpuskularstrahlen durch Materie". Annalen der Physik (in German). 397 (3): 325–400. Bibcode:1930AnP...397..325B. doi:10.1002/andp.19303970303.
  24. ^ Schweber 2012, p. 181.
  25. ^ Brown & Lee 2006, p. 7.
  26. ^ Schweber 2012, pp. 182–183.
  27. ^ Schweber 2012, p. 187.
  28. ^ Corlin, Axel; Stein, J. S.; Beck, G.; Bethe, H.; Riezler, W. (1931). "Zuschriften". Die Naturwissenschaften. 19 (2): 37. Bibcode:1931NW.....19...37C. doi:10.1007/BF01523870.
  29. ^ Schweber 2012, pp. 190–192.
  30. ^ Schweber 2012, p. 193.
  31. ^ Schweber 2012, pp. 199–202.
  32. ^ Schweber 2012, p. 195.
  33. ^ a b Schweber 2012, pp. 202–208.
  34. ^ Bernstein 1980, p. 32.
  35. ^ Schweber 2012, pp. 211, 220–221.
  36. ^ Bernstein 1980, p. 33.
  37. ^ Schweber 2012, pp. 223–224.
  38. ^ a b Bernstein 1980, p. 35.
  39. ^ Schweber 2012, pp. 237–240.
  40. ^ a b Schweber 2012, p. 244.
  41. ^ Chadwick, J.; Goldhaber, M. (1934). "A 'Nuclear Photo-effect': Disintegration of the Diplon by γ-Rays". Nature. 134 (3381): 237. Bibcode:1934Natur.134..237C. doi:10.1038/134237a0.
  42. ^ Brown & Lee 2009, p. 9.
  43. ^ Schweber 2012, pp. 262–263.
  44. ^ Schweber 2012, pp. 272–275.
  45. ^ Schweber 2012, p. 279.
  46. ^ Brown & Lee 2006, p. 136.
  47. ^ a b Schweber 2012, pp. 296–298.
  48. ^ Schweber 2012, pp. 305–307.
  49. ^ Bethe, H.; Bacher, R (1936). "Nuclear Physics. A: Stationary States of Nuclei". Reviews of Modern Physics. 8 (2): 82–229. Bibcode:1936RvMP....8...82B. doi:10.1103/RevModPhys.8.82.
  50. ^ Bethe, H. (1937). "Nuclear Physics. B: Nuclear Dynamics, Theoretical". Reviews of Modern Physics. 9 (2): 69–244. Bibcode:1937RvMP....9...69B. doi:10.1103/RevModPhys.9.69.
  51. ^ Bethe, H.; Livingston, M. S. (1937). "Nuclear Physics. C: Nuclear Dynamics, Experimental". Reviews of Modern Physics. 9 (2): 245–390. Bibcode:1937RvMP....9..245L. doi:10.1103/RevModPhys.9.245.
  52. ^ Brown & Lee 2009, p. 11.
  53. ^ Schweber 2012, p. 313.
  54. ^ Schweber 2012, p. 370.
  55. ^ a b Bernstein 1980, pp. 45–47.
  56. ^ Schweber 2012, pp. 345–347.
  57. ^ Schweber 2012, p. 347.
  58. ^ Schweber 2012, pp. 348–350.
  59. ^ a b Schweber 2012, pp. 351–352.
  60. ^ Bernstein 1980, p. 39.
  61. ^ Bernstein 1980, pp. 51–52.
  62. ^ Brown & Lee 2006, p. 149.
  63. ^ Bernstein 1980, pp. 54–55.
  64. ^ a b "Hans Bethe – Biographical". The Nobel Foundation. Retrieved July 7, 2013.
  65. ^ Truscott, Alan. "Bridge: Son of Nobel Prize Winner Is Famed in His Own Right". The New York Times. February 24, 1988. Retrieved April 11, 2015.
  66. ^ Schweber 2012, p. 382.
  67. ^ Brown & Lee 2006, p. 143.
  68. ^ Bernstein 1980, p. 61.
  69. ^ Brown & Lee 2009, pp. 13–14.
  70. ^ Brown & Lee 2009, p. 13.
  71. ^ Hoddeson et al. 1993, pp. 42–47.
  72. ^ a b Weil, Martin (March 8, 2005). "Hans Bethe Dies; Nobel Prize Winner Worked on A-Bomb". The Washington Post. p. B06.
  73. ^ Hoddeson et al. 1993, pp. 92–83.
  74. ^ Szasz 1992, pp. 19–20.
  75. ^ Hoddeson et al. 1993, pp. 204, 246.
  76. ^ Hoddeson et al. 1993, pp. 179–184.
  77. ^ Hoddeson et al. 1993, p. 129.
  78. ^ Hoddeson et al. 1993, pp. 308–310.
  79. ^ Hoddeson et al. 1993, pp. 344–345.
  80. ^ Peplow, Mark (March 8, 2005). "Hans Bethe – Nuclear physicist dies at 98". Nature. doi:10.1038/news050307-7.
  81. ^ Bernstein 1980, pp. 92–96.
  82. ^ a b Schweber 2000, p. 166.
  83. ^ Bernstein 1980, pp. 97–99.
  84. ^ a b Brown & Lee 2006, pp. 157–158.
  85. ^ Brown & Lee 2009, p. 15.
  86. ^ H. Bethe (1947). "The Electromagnetic Shift of Energy Levels". Physical Review. 72 (4): 339–341. Bibcode:1947PhRv...72..339B. doi:10.1103/PhysRev.72.339.
  87. ^ Brown & Lee 2006, pp. 158–159.
  88. ^ Alpher, R. A.; Bethe, H.; Gamow, G. (1 April 1948). "The Origin of Chemical Elements" (PDF). Physical Review. 73 (7): 803–804. Bibcode:1948PhRv...73..803A. doi:10.1103/PhysRev.73.803. Archived from the original (PDF) on 8 July 2013. Retrieved March 10, 2011.
  89. ^ Bernstein 1980, p. 46.
  90. ^ Brown & Lee 2006, pp. 165–171.
  91. ^ "Hans A. Bethe Prize winners". American Physical Society. Retrieved July 7, 2013.
  92. ^ Brown & Lee 2006, pp. 176–180.
  93. ^ Brown & Lee 2006, pp. 151–153.
  94. ^ Bahcall, J.N.; Bethe, H.A. (1990). "A solution of the solar neutrino problem". Physical Review Letters. 65 (18): 2233–2235. Bibcode:1990PhRvL..65.2233B. doi:10.1103/PhysRevLett.65.2233.
  95. ^ Brown & Lee 2006, p. 182.
  96. ^ Bethe, Hans A.; Brown, G. E. (1998). "Evolution of Binary Compact Objects That Merge". Astrophysical Journal. 506 (2): 780–789. arXiv:astro-ph/9802084. Bibcode:1998ApJ...506..780B. doi:10.1086/306265.
  97. ^ Garwin, R. L.; Bethe, H.A. (March 1968). "Anti-Ballistic Missile Systems". Scientific American. 218 (3): 21–31. Bibcode:1968SciAm.218c..21G. doi:10.1038/scientificamerican0368-21.
  98. ^ Bernstein 1980, pp. 107–112.
  99. ^ Rhodes, Richard. "Chernobyl". PBS. Retrieved July 6, 2013.
  100. ^ Brown & Lee 2006, p. 266.
  101. ^ Bethe 1991, pp. 113–131.
  102. ^ "Hans Albrecht Bethe". Nuclear Age Peace Foundation. Retrieved July 6, 2013.
  103. ^ "48 Nobel Winning Scientists Endorse Kerry-June 21, 2004". George Washington University. Retrieved July 6, 2013.
  104. ^ Herken 2002, p. 334.
  105. ^ Schweber 2012, p. 44.
  106. ^ Brown & Lee 2006, pp. 126–128.
  107. ^ Nobel Laureate Hans Bethe passes away at age of 98, March 7, 2005, Wikinews
  108. ^ Tucker, Anthony (March 8, 2005). "Obituary: Hans Bethe". The Guardian.
  109. ^ "Hans Bethe". Array of Contemporary Physicists. Archived from the original on August 30, 2010. Retrieved July 7, 2013.
  110. ^ "Book of Members, 1780–2010: Chapter B" (PDF). American Academy of Arts and Sciences. Retrieved June 24, 2011.
  111. ^ "Henry Draper Medal". National Academy of Sciences. Archived from the original on July 22, 2012. Retrieved February 24, 2011.
  112. ^ Brown & Lee 2009, p. 17.
  113. ^ "Past Recipients of the Rumford Prize". American Academy of Arts and Sciences. Archived from the original on September 27, 2012. Retrieved February 24, 2011.
  114. ^ "The President's national Medal of Science". National Science Foundation.
  115. ^ "Oersted Medal". Retrieved July 7, 2013.
  116. ^ "Past Winners of the Catherine Wolfe Bruce Gold Medal". Astronomical Society of the Pacific. Retrieved 24 February 2011.
  117. ^ "Benjamin Franklin Medal for Distinguished Achievement in the Sciences Recipients". American Philosophical Society. Retrieved November 26, 2011.
  118. ^ Bethe, Hans A. (1994). "Mechanism of Supernovae". Philos. Trans. R. Soc. Lond. A 346: 251–258.
  119. ^ "List of Members". www.leopoldina.org. Retrieved 8 October 2017.
  120. ^ "Hans Bethe House". Cornell University. Retrieved July 7, 2013.
  121. ^ "Council for a Livable World, Our Legacy". Retrieved July 7, 2013.
  122. ^ "Bethe Center for Theoretical Physics". Retrieved July 7, 2013.
  123. ^ "JPL Small-Body Database Browser on 30828 Bethe". NASA. Retrieved July 7, 2013.
  124. ^ "Hans A. Bethe Prize Prize for astrophysics, nuclear physics, nuclear astrophysics and related fields". American Physical Society. Retrieved July 7, 2013.

References

  • Bernstein, Jeremy (1980). Hans Bethe, Prophet of Energy. New York: Basic Books. ISBN 978-0-465-02903-7.
  • Bethe, Hans A. (1991). The Road from Los Alamos. New York: American Institute of Physics. ISBN 978-0-88318-707-4.
  • Brian, Denis (2001). The Voice Of Genius: Conversations With Nobel Scientists And Other Luminaries. Cambridge, Massachusetts: Perseus Pub. ISBN 978-0-7382-0447-5.
  • Brown, Gerald E.; Lee, Sabine (2009). Hans Albrecht Bethe (PDF). Biographical Memoirs. Washington, D.C.: National Academy of Sciences.
  • Brown, Gerald E.; Lee, Chang-Hwan, eds. (2006). Hans Bethe and his Physics. New Jersey: World Scientific Publishing. ISBN 9812566090.
  • Herken, Gregg (2002). Brotherhood of the Bomb: The Tangled Lives and Loyalties of Robert Oppenheimer, Ernest Lawrence, and Edward Teller. New York: Henry Holt and Company. ISBN 0-8050-6588-1.
  • Hoddeson, Lillian; Henriksen, Paul W.; Meade, Roger A.; Westfall, Catherine L. (1993). Critical Assembly: A Technical History of Los Alamos During the Oppenheimer Years, 1943–1945. New York: Cambridge University Press. ISBN 0-521-44132-3. OCLC 26764320.
  • Schweber, Silvan S. (2000). In the Shadow of the Bomb: Bethe, Oppenheimer, and the Moral Responsibility of the Scientist. Princeton: Princeton University Press. ISBN 978-0-691-04989-2.
  • Schweber, Silvan S. (2012). Nuclear Forces: The Making of the Physicist Hans Bethe. Cambridge, Massachusetts: Harvard University Press. ISBN 978-0-674-06587-1.
  • Szasz, Ferenc Morton (1992). British Scientists and the Manhattan Project: the Los Alamos Years. New York: St. Martin's Press. ISBN 978-0-312-06167-8. OCLC 23901666.

External links

Albrecht Bethe

Albrecht Julius Theodor Bethe (25 April 1872 in Stettin – 19 October 1954 in Frankfurt am Main) was a German physiologist. He was the father of physicist Hans Bethe (1906–2005).

He studied at the universities of Freiburg, Munich (under Richard Hertwig), Berlin and Strasbourg (under Friedrich Goltz and Ernst Julius Richard Ewald); receiving his PhD in 1895 at Munich. From 1896 to 1911 he worked at the institute of physiology in Strasbourg, where in 1898 he obtained his doctorate in medicine. In 1911 he became a professor of physiology at the University of Kiel, and four years later, relocated as a professor to the University of Frankfurt. In 1937 he was relieved of his professorial duties at Frankfurt (his wife was deemed to be half-Jewish by the Nazis), only to have them reinstated following the end of wartime hostilities in Europe.He is well known for his studies involving the nervous system of invertebrates. He believed in the "plasticity" of the nervous system, asserting that if one part of the brain is damaged, another part could learn the functions of the damaged portion.He was a co-editor of "Pflüger's Archiv für die gesamte Physiologie" (from 1918 onward) and of the "Handbuch der normalen und pathologischen Physiologie" (1925–32).

Bethe

Bethe is a surname and a given name which may refer to:

Albrecht Bethe (1872–1954), German physiologist and father of Hans Bethe

Erich Bethe (1863–1940), German philologist

Hans Bethe (1906–2005), German-American nuclear physicist

Kitty Cooper (born 1960), American bridge player also known as Kitty Bethe

Bethe Correia (born 1983), Brazilian mixed martial artist

Bethe ansatz

In physics, the Bethe ansatz is an ansatz method for finding the exact solutions of certain one-dimensional quantum many-body models. It was invented by Hans Bethe in 1931 to find the exact eigenvalues and eigenvectors of the one-dimensional antiferromagnetic Heisenberg model Hamiltonian. Since then the method has been extended to other models in one dimension: Bose gas, Hubbard model, etc.

Bethe formula

The Bethe formula describes the mean energy loss per distance travelled of swift charged particles (protons, alpha particles, atomic ions) traversing matter (or alternatively the stopping power of the material). For electrons the energy loss is slightly different due to their small mass (requiring relativistic corrections) and their indistinguishability, and since they suffer much larger losses by Bremsstrahlung, terms must be added to account for this. Fast charged particles moving through matter interact with the electrons of atoms in the material. The interaction excites or ionizes the atoms, leading to an energy loss of the traveling particle.

The non-relativistic version was found by Hans Bethe in 1930; the relativistic version (shown below) was found by him in 1932. The most probable energy loss differs from the mean energy loss and is described by the Landau-Vavilov distribution.The Bethe formula is sometimes called "Bethe-Bloch formula", but this is misleading (see below).

Bethe lattice

A Bethe lattice, introduced by Hans Bethe in 1935, is an infinite connected cycle-free graph where each node is connected to z neighbours, where z is called the coordination number. It is a rooted tree, with all other nodes arranged in shells around the root node, also called the origin of the lattice. The number of nodes in the kth shell is given by

In some situations the definition is modified to specify that the root node has z − 1 neighbors.

Due to its distinctive topological structure, the statistical mechanics of lattice models on this graph are often exactly solvable. The solutions are related to the often used Bethe approximation for these systems.

Since this is a cycle free graph, every vertex connects from the caley tree to a new node, then the average connectivity of each particle c is given by

Bethe–Feynman formula

The Bethe–Feynman efficiency formula, a simple method for calculating the yield of a fission bomb, was first derived in 1943 after development in 1942. Aspects of the formula are speculated to be secret restricted data.

CNO cycle

The CNO cycle (for carbon–nitrogen–oxygen) is one of the two known sets of fusion reactions by which stars convert hydrogen to helium, the other being the proton–proton chain reaction (pp-chain reaction). Unlike the latter, the CNO cycle is a catalytic cycle. It is dominant in stars that are more than 1.3 times as massive as the Sun.In the CNO cycle, four protons fuse, using carbon, nitrogen, and oxygen isotopes as catalysts, to produce one alpha particle, two positrons and two electron neutrinos. Although there are various paths and catalysts involved in the CNO cycles, all these cycles have the same net result:

4 11H + 2 e− → 42He + 2 e+ + 2 e− + 2 νe + 3 γ + 24.7 MeV → 42He + 2 νe + 3 γ + 26.7 MeVThe positrons will almost instantly annihilate with electrons, releasing energy in the form of gamma rays. The neutrinos escape from the star carrying away some energy. One nucleus goes on to become carbon, nitrogen, and oxygen isotopes through a number of transformations in an endless loop.

The proton–proton chain is more prominent in stars the mass of the Sun or less. This difference stems from temperature dependency differences between the two reactions; pp-chain reaction starts at temperatures around 4×106 K (4 megakelvin), making it the dominant energy source in smaller stars. A self-maintaining CNO chain starts at approximately 15×106 K, but its energy output rises much more rapidly with increasing temperatures so that it becomes the dominant source of energy at approximately 17×106 K.

The Sun has a core temperature of around 15.7×106 K, and only 1.7% of 4He nuclei produced in the Sun are

born in the CNO cycle. The CNO-I process was independently proposed by Carl von Weizsäcker and Hans Bethe in the late 1930s.

Cornell West Campus

West Campus is a residential section of Cornell University's Ithaca, New York campus located west of Libe Slope and between the Fall Creek gorge and the Cascadilla gorge. It now primarily houses transfer students, second year, and upperclassmen.

Crystal field theory

Crystal Field Theory (CFT) is a model that describes the breaking of degeneracies of electron orbital states, usually d or f orbitals, due to a static electric field produced by a surrounding charge distribution (anion neighbors). This theory has been used to describe various spectroscopies of transition metal coordination complexes, in particular optical spectra (colors). CFT successfully accounts for some magnetic properties, colors, hydration enthalpies, and spinel structures of transition metal complexes, but it does not attempt to describe bonding. CFT was developed by physicists Hans Bethe and John Hasbrouck van Vleck in the 1930s. CFT was subsequently combined with molecular orbital theory to form the more realistic and complex ligand field theory (LFT), which delivers insight into the process of chemical bonding in transition metal complexes.

Foe (unit)

A foe is a unit of energy equal to 1044 joules or 1051 ergs, used to express the large amount of energy released by a supernova. The word is an acronym derived from a part of the pronunciation "ten to the power of fifty-one ergs".It was coined by Gerald E. Brown of Stony Brook University in his work with Hans Bethe, because "it came up often enough in our work". A bethe (B) is equivalent to a foe. The bethe is named after Hans Bethe. It was coined by Steven Weinberg.This unit of measure is convenient because a supernova typically releases about one foe of observable energy in a very short period (which can be measured in seconds). In comparison, if the Sun had its current luminosity throughout its entire lifetime, it would release 3.827×1026 W × 3.1536×107 s/yr × 1010 yr ≈ 1.2 foe. One solar mass has a rest mass energy of 1787 foe.

George Placzek

George Placzek (native name: Georg Placzek) (September 26, 1905 – October 9, 1955) was a Czech physicist.Placzek was born in Brno, Moravia, then part of Austria-Hungary, into a wealthy Jewish family. He studied physics in Prague and Vienna. In the 1930s, Placzek was known as an adventurous person with sharp sense of humor, a tireless generator of novel physics ideas which he generously shared with his colleagues. The scope of Placzek's pilgrimage around world's physics centers in the 1930s was unique among his colleagues. He worked with Hans Bethe, Edward Teller, Rudolf Peierls, Werner Heisenberg, Victor Weisskopf, Enrico Fermi, Niels Bohr, Lev Landau, Edoardo Amaldi, Emilio Segrè, Otto Frisch, Leon van Hove and many other prominent physicists of his time. His wife, Els Placzek (née Andriesse) was an ex-wife of physicist Hans von Halban. He lost all his relatives to Holocaust, casting a tragic shadow on his life. Placzek's major areas of scientific work involved a fundamental theory of Raman scattering, molecular spectroscopy in gases and liquids, neutron physics and mathematical physics. Together with Otto Frisch, he suggested a direct experimental proof of nuclear fission. Together with Niels Bohr and others, he was instrumental in clarifying the role of Uranium 235 for the possibility of nuclear chain reaction.During his stay in Landau's circle in Kharkiv around 1937, Placzek witnessed the brutal reality of Joseph Stalin's regime. His first-hand experience of this influenced the political opinions of his close friends, in particular, fathers of nuclear and thermonuclear bombs, Robert Oppenheimer and Edward Teller. Later, Placzek was the only Czech with a leading position in the Manhattan project, where he worked from 1943 till 1946 as a member of the British Mission; first in Canada as the leader of a theoretical division at the Montreal Laboratory and then (since May 1945) in Los Alamos, later replacing his friend Hans Bethe as the leader of the theoretical group. Since 1948, Placzek was a member of the Institute for Advanced Study in Princeton, USA.

Unlike many trailblazers of nuclear physics, George Placzek did not leave his recollections or life story notes. Many new facts about Placzek's life and his family roots emerged in connection with a Symposium held in Placzek's memory.

Placzek's premature death in a hotel in Zurich was very likely a suicide influenced by his long-time serious illness. The first detailed biography of George Placzek sheds light on poorly known pages of his life, illuminating also circumstances of Placzek's death.

Hans Bethe Prize

The Hans A. Bethe Prize, is presented annually by the American Physical Society.

The prize honors outstanding work in theory, experiment or observation in the areas of astrophysics, nuclear physics, nuclear astrophysics, or closely related fields. The prize consists of $10,000 and a certificate citing the contributions made by the recipient.

Hans Bethe prize is endowed by contributions from the Division of Astrophysics, the Division of Nuclear Physics and friends of the Nobel laureate Hans A. Bethe to honor him for his outstanding and numerous accomplishments in both astrophysics and nuclear physics.

The prize has been awarded annually since 1998.

Kelvin–Helmholtz mechanism

The Kelvin–Helmholtz mechanism is an astronomical process that occurs when the surface of a star or a planet cools. The cooling causes the pressure to drop, and the star or planet shrinks as a result. This compression, in turn, heats the core of the star/planet. This mechanism is evident on Jupiter and Saturn and on brown dwarfs whose central temperatures are not high enough to undergo nuclear fusion. It is estimated that Jupiter radiates more energy through this mechanism than it receives from the Sun, but Saturn might not. The latter process causes Jupiter to shrink at a rate of two centimetres each year.The mechanism was originally proposed by Kelvin and Helmholtz in the late nineteenth century to explain the source of energy of the Sun. By the mid-nineteenth century, conservation of energy had been accepted, and one consequence of this law of physics is that the Sun must have some energy source to continue to shine. Because nuclear reactions were unknown, the main candidate for the source of solar energy was gravitational contraction.

However, it soon was recognized by Sir Arthur Eddington and others that the total amount of energy available through this mechanism only allowed the Sun to shine for millions of years rather than the billions of years that the geological and biological evidence suggested for the age of the Earth. (Kelvin himself had argued that the Earth was millions, not billions, of years old.) The true source of the Sun's energy remained uncertain until the 1930s, when it was shown by Hans Bethe to be nuclear fusion.

List of Cornell Manhattan Project people

Scientists from Cornell University played a major role in developing the technology that resulted in the first atomic bombs used in World War II. In turn, Cornell Physics professor Hans Bethe used the project as an opportunity to recruit young scientists to join the Cornell faculty after the war. The following people worked on the Manhattan Project primarily in Los Alamos, New Mexico during World War II and either studied or taught at Cornell University before or after the War:

Robert Fox Bacher – headed the experimental physics division, Cornell Physics professor from 1935 until the War

Manson Benedict – developed the gaseous diffusion method for separating the isotopes of uranium and supervised the engineering and process development of the K-25 plant in Oak Ridge, Tennessee, where fissionable material for the atomic bomb was produced

Hans Bethe – director of the theoretical division

Gertrude Blanch – oversaw calculations for the Manhattan Project

Oswald C. Brewster – Cornell class of 1918, project engineer who wrote to senior government officials warning about the potential of atomic bombs ending civilization.

Walter S. Carpenter, Jr. – oversaw the DuPont company's involvement in the Manhattan Project

Frederick J. Clarke – master's degree in civil engineering from Cornell University in 1940

Dale R. Corson – later became President of Cornell

John Curtin – Cornell theoretical physics Ph.D class of 1943

Jean Klein Dayton – helped design detonation systems

John W. DeWire – Cornell physics faculty

Richard Davisson – worked in Special Engineer Detachment

Eleanor & Richard Ehrlich

Richard Feynman – team leader under Bethe, later taught Physics at Cornell

Kenneth Greisen – worked on instrumentation, later Cornell Physics faculty

Lottie Grieff

William Higinbotham – headed the electronics group

Marshall Holloway – PhD from Cornell

Henry Hurwitz, Jr. – Cornell class of 1938

Walter Kauzmann – in charge of producing the detonator for the Trinity test

Margaret Ramsey Keck

Giovanni Rossi Lomanitz – worked at the Berkeley Radiation Laboratory; doctorate in theoretical physics from Cornell University, where he was the first graduate student of Richard Feynman.

Robert Marshak – PhD from Cornell University in 1939

Boyce McDaniel – later became director of Cornell's Laboratory of Nuclear Studies

William T. Miller – developed the chlorofluorocarbon polymer used in the first gaseous diffusion plant for the separation of uranium isotopes, Cornell chemistry faculty, 1936 – 1977

Elliott Waters Montroll – Head of the Mathematics Research Group at the Kellex Corporation in New York, working on programs associated with the Manhattan Project.

Philip Morrison – Cornell physics faculty 1946 – 1964.

Kenneth Nichols – deputy to General Leslie Groves, ME from Cornell

Paul Olum – later became President of the University of Oregon

Lyman G. Parrett – Cornell physics faculty

Arthur V. Peterson – Manhattan District's Chicago Area Engineer, responsible for the Metallurgical Laboratory

Edith Hinkley Quimby

Marcia White Rosenthal

Bruno Rossi – co-director of the Detector Group, Cornell physics faculty 1942-1946

Harvey L. Slatin – physicist and inventor who worked on the isolation of plutonium with the Special Engineering Detachment

LaRoy Thompson – Cornell class of 1942, physically assembled the first bomb and flew the practice bombing run at Bikini Island. Later, senior vice president and treasurer of the University of Rochester

Robert R. Wilson – head of the Cyclotron Group (R-1)

William M. Woodward – Cornell physics faculty

Mark Nelkin

Mark Samuel Nelkin is a theoretical physicist at the Cornell University.

Under the direction of Professor Hans Bethe, he received his Ph.D. in theoretical physics from Cornell in 1955. He was awarded a Guggenheim Fellowship in 1968.He became a Fellow of the American Physical Society in 1984, having been nominated by their Division of Fluid Dynamics, for contributions to the advancement of physics by strong theoretical contributions in four areas beginning with the physics of thermal neutrons and its applications to nuclear reactors, kinetic theory of fluctuations in fluids, turbulence, and 1/f noise.

Nelkin was married to American sociologist of science Dorothy Nelkin until her death in 2003.

Mikheyev–Smirnov–Wolfenstein effect

The Mikheyev–Smirnov–Wolfenstein effect (often referred to as matter effect) is a particle physics process which can act to modify neutrino oscillations in matter. Works in 1978 and 1979 by American physicist Lincoln Wolfenstein led to understanding that the oscillation parameters of neutrino are changed in matter. In 1985, the Soviet physicists Stanislav Mikheyev and Alexei Smirnov predicted that slow decrease of the matter density can resonantly enhance the neutrino mixing. Later in 1986, Stephen Parke of Fermilab, Hans Bethe of Cornell University, and S. Peter Rosen and James Gelb of Los Alamos National Laboratory provided analytic treatments of this effect.

Oersted Medal

The Oersted Medal recognizes notable contributions to the teaching of physics. Established in 1936, it is awarded by the American Association of Physics Teachers. The award is named for Hans Christian Ørsted. It is the Association's most prestigious award.

Well-known recipients include Nobel laureates Robert Andrews Millikan, Edward M. Purcell, Richard Feynman, Isidor I. Rabi, Norman F. Ramsey, Hans Bethe, and Carl Wieman; as well as Arnold Sommerfeld, George Uhlenbeck, Jerrold Zacharias, Philip Morrison, Melba Phillips, Victor Weisskopf, Gerald Holton, John A. Wheeler, Frank Oppenheimer, Robert Resnick, Carl Sagan, Freeman Dyson, Daniel Kleppner, and Lawrence Krauss, and Anthony French, David Hestenes, Robert Karplus, Robert Pohl, and Francis Sears.

The 2008 medalist, Mildred S. Dresselhaus, is the third woman to win the award in its 70-plus-year history.

Roswell Clifton Gibbs

Roswell Clifton Gibbs (July 1, 1878 – October 4, 1966) was Chairman of the Department of Physics at Cornell University from 1934 to 1946. A graduate of Cornell, he became an assistant professor of Physics there in 1912, and a professor in 1918. His research primarily concerned spectroscopy, and he was the author or co-author of over forty research papers. As Chairman of the Department of Physics, he hired distinguished physicists including Stanley Livingston, Robert Bacher and Hans Bethe, who later won the Nobel Prize in Physics for his work at Cornell. After World War II, Gibbs was Chairman of the Mathematical and Physical Sciences Division of the National Research Council.

Wolfgang Paul

Wolfgang Paul (10 August 1913 – 7 December 1993) was a German physicist, who co-developed the non-magnetic quadrupole mass filter which laid the foundation for what is now called an ion trap. He shared one-half of the Nobel Prize in Physics in 1989 for this work with Hans Georg Dehmelt; the other half of the Prize in that year was awarded to Norman Foster Ramsey, Jr.

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