Mário Schenberg
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Mário Schenberg | |
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Schönberg-Chandrasekhar limit Urca process | |
Scientific career | |
Fields | Theoretical physics |
Doctoral students | José Leite Lopes |
Notes | |
Brazilian physicist of the 'heroic era' (1900–1945), together with Cesar Lattes, Jayme Tiomno, and Joaquim da Costa Ribeiro . |
Mário Schenberg (born Mayer Schönberg [var. Mário Schönberg, Mario Schonberg, Mário Schoenberg]; 2 July 1914 – 10 November 1990) was a Brazilian
Early life
Schenberg was born in
Scientific work
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The Urca process
Widely regarded as one of Brazil's most important theoretical physicists, Schenberg is best remembered for his contributions to astrophysics, particularly the theory of nuclear processes in the formation of supernova stars. He provided the inspiration for the name of the so-called Urca process, a cycle of nuclear reactions in which a nucleus loses energy by absorbing an electron and then re-emitting a beta particle plus a neutrino-antineutrino pair, leading to the loss of internal supporting pressure and consequent collapse and explosion in the form of a supernova. George Gamow (1904–1968) was inspired to name the process Urca after the name of a casino in Rio de Janeiro, when Schenberg remarked to him that "the energy disappears in the nucleus of the supernova as quickly as the money disappeared at that roulette table".
Schönberg–Chandrasekhar limit
Together with Indian physicist Subrahmanyan Chandrasekhar (1910–1995), he discovered and published in 1942 the so-called Schönberg–Chandrasekhar limit, which is the maximum mass of the core of a star that can support the overlying layers against gravitational collapse, once the core hydrogen is exhausted.
Quantum physics and geometric algebra
In the University of São Paulo had Schönberg interacted closely with David Bohm during the final years of Bohm's exile in Brazil,[1] and, in 1954, Schönberg demonstrated a link among the quantized motion of the Madelung fluid and the trajectories of the de Broglie–Bohm theory.[2]
He wrote a series of publications of 1957/1958 on
His work has been cited, together with that of Marcel Riesz, for its importance to Clifford algebras and mathematical physics in the proceedings of a workshop held in France in 1989 which had been dedicated to these two mathematicians.[7]
Politics and life
Schenberg was a member of the Brazilian Communist Party[8][9] and professor of the University of São Paulo.
Articles
His articles include:
- M. Schönberg: Quantum kinematics and geometry, Il Nuovo Cimento (1955–1965), vol. 6, Supplement 1, pp. 356–380, 1957, )
- M. Schönberg, S. Chandrasekhar: On the Evolution of the Main-Sequence Stars, Astrophysical Journal, vol. 96, no. p. 161 ff., 1942, fulltext
Legacy
- Mario Schenberg Graviton, a spherical, resonant-mass, gravitational wave detector.
References
- ^ Olival Freireon January 11, 2008, Oral History Transcript, Niels Bohr Library & Archives, American Institute of Physics
- )
- ^ a b F. A. M. Frescura, B. J. Hiley: Algebras, quantum theory and pre-space, p. 3–4 (published in Revista Brasileira de Fisica, Volume Especial, Julho 1984, Os 70 anos de Mario Schonberg, pp. 49–86)
- ^ M. Schönberg, Quantum mechanics and geometry, An. Acad. Brasil. Cien., 30, pp. 1–20, 1958. Cited after: F. A. M. Frescura, B. J. Hiley: Algebras, quantum theory and pre-space, p. 3–4 (published in Revista Brasileira de Fisica, Volume Especial, Julho 1984, Os 70 anos de Mario Schonberg, pp. 49–86)
- ^ B. J. Hiley: A note on the role of idempotents in the extended Heisenberg algebra, "Implications", Scientific Aspects of ANPA 22, pp. 107–121, Cambridge, UK, 2001.
- ), therein p. 201
- ISBN 0-7923-1623-1, Foreword(in French language)
- ISBN 9780230339613.
- ISSN 0103-4014. Retrieved 7 December 2015.