Hans Bethe: Difference between revisions
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<p style="margin-left: 2.0%; margin-right: 6%; font-size: 1.0em; font-family: Trebuchet MS;">If all this is true, stars have a life cycle much like animals. They get born, they grow, they go through a definite internal development, and finally they die, to give back the material of which they are made so that new stars may live.<ref name=bethelect>Hans Bethe. [http://nobelprize.org/nobel_prizes/physics/laureates/1967/bethe-lecture.html Energy Production in Stars] The Nobel Prize in Physics 1967. Nobel Lecture, December 11, 1967.</ref></p> | <p style="margin-left: 2.0%; margin-right: 6%; font-size: 1.0em; font-family: Trebuchet MS;">If all this is true, stars have a life cycle much like animals. They get born, they grow, they go through a definite internal development, and finally they die, to give back the material of which they are made so that new stars may live.<ref name=bethelect>Hans Bethe. [http://nobelprize.org/nobel_prizes/physics/laureates/1967/bethe-lecture.html Energy Production in Stars] The Nobel Prize in Physics 1967. Nobel Lecture, December 11, 1967.</ref></p> | ||
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During World War II, he headed the theoretical physics division at Los Alamos, New Mexico, where he contributed to the development of the first atomic bomb. | |||
==Life and work== | ==Life and work== | ||
Revision as of 18:20, 30 December 2008
His life nearly spanning the 20th century and productively extending into the 21st, Hans Bethe (1906-2005), née Hans Albrecht Bethe, earned a position in the highest rank of pioneer physicists of the 20th century. [1] [2] [3] He devoted much of intellectual energy in helping develop the theory of atomic nuclei and of nuclear reactions. That work led him to discover the reactions in the sun that delivers energy to its surrounding, including Earth, for which discovery, and for his discovery of the different set of nuclear reactions that generates the radiant energy of stars more massive than the sun, and for his many contributions to the theory of nuclear reactions, he received the Nobel Prize in Physics in 1967, as sole recipient. He concluded his Nobel Lecture as follows:
If all this is true, stars have a life cycle much like animals. They get born, they grow, they go through a definite internal development, and finally they die, to give back the material of which they are made so that new stars may live.[4]
During World War II, he headed the theoretical physics division at Los Alamos, New Mexico, where he contributed to the development of the first atomic bomb.
Life and work
Han Bethe joined humanity in Strasbourg, Alsace-Lorraine, born on July 2, 1906, and died in Ithaca, New York, on March 6, 2005, leaving humanity with a invaluable legacy of knowledge about the nature of the universe and of humanity itself.
References and notes cited in text
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- ↑ Biography: Hans Bethe, The Nobel Prize in Physics 1967.
- Excerpt: Bethe's main work is concerned with the theory of atomic nuclei. Together with Peierls, he developed a theory of the deuteron in 1934 which he extended in 1949. He resolved some contradictions in the nuclear mass scale in 1935. He studied the theory of nuclear reactions in 1935-1938, predicting many reaction cross sections. In connection with this work, he developed Bohr's theory of the compound nucleus in a more quantitative fashion. This work and also the existing knowledge on nuclear theory and experimental results, was summarized in three articles in the Reviews of Modern Physics which for many years served as a textbook for nuclear physicists.
- ↑ Biography from Los Alamos National Laboratory
- Excerpt: Over the winter of 1942-43, Project Y came together at Los Alamos under the leadership of General Leslie R. Groves and Oppenheimer. Hans Bethe emerged as a primary candidate to work at the Los Alamos project. Edward Teller, his old friend and Berkeley summer colleague, urged an ambivalent Bethe to join the project. Bethe finally gave in, and Oppenheimer made him chief of the Theoretical Division, a position Teller sorely coveted. This slight marked the beginning of a feud that would last for decades.
- ↑ About Hans Bethe. From website: Quantum Physics Made Relatively Simple: Personal and Historical Perspectives of Hans Bethe 2004. Last accessed: December 30, 2008.
- Excerpt: In the decade following World War II, Bethe and Feynman and their students played a central role in developing quantum electrodynamics, work for which Feynman shared the Nobel Prize. From 1945, until his retirement from the Cornell faculty in 1975, Bethe trained and inspired a large number of graduate students. Many have gone on to become internationally known scientists, among them Freeman Dyson. Bethe and his co-workers published important work across the whole spectrum of physics. Even today, in his nineties, his unique mastery of such diverse subjects as thermonuclear processes, shock waves and neutrino reactions have kept Bethe at the forefront of research in astrophysics.
- ↑ Hans Bethe. Energy Production in Stars The Nobel Prize in Physics 1967. Nobel Lecture, December 11, 1967.