Biography:Hans Bethe: Difference between revisions
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{{Infobox person | {{Infobox person | ||
| name = Hans Bethe | | name = Hans Bethe | ||
| image = Hans Bethe portrait.jpg | |||
| caption = Hans Bethe | |||
| fields = Physics | | fields = Physics | ||
| known_for = Hans Albrecht Eduard Bethe (; German: ˈhans ˈbeːtə ; 2 July 1906 – 6 March 2005) was a German-American physicist who made major contributions to nuclear physics, astrophysics, quantum electrodynamics and. | | known_for = Hans Albrecht Eduard Bethe (; German: ˈhans ˈbeːtə ; 2 July 1906 – 6 March 2005) was a German-American physicist who made major contributions to nuclear physics, astrophysics, quantum electrodynamics and. | ||
Revision as of 20:37, 24 May 2026
| Hans Bethe | |
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| Hans Bethe
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| Fields | Physics |
| Known for | Hans Albrecht Eduard Bethe (; German: ˈhans ˈbeːtə ; 2 July 1906 – 6 March 2005) was a German-American physicist who made major contributions to nuclear physics, astrophysics, quantum electrodynamics and. |
Hans Bethe is a biographical subject in the ScholarlyWiki science collection. Hans Albrecht Eduard Bethe (; German: ˈhans ˈbeːtə ; 2 July 1906 – 6 March 2005) was a German-American physicist who made major contributions to nuclear physics, astrophysics, quantum electrodynamics and solid-state physics, and received the Nobel Prize in Physics in 1967 for his work on the theory of stellar nucleosynthesis. For most of his career, Bethe was a professor at Cornell University.[1]
Work and context
In 1931, Bethe developed the Bethe ansatz, which is a method for finding the exact solutions for the eigenvalues and eigenvectors of certain one-dimensional quantum many-body models. In 1939, Bethe published a paper which established the CNO cycle as the primary energy source for heavier stars in the main sequence classification of stars, which earned him a Nobel Prize in 1967.
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References
- ↑ "Hans Bethe". Wikipedia. https://en.wikipedia.org/wiki/Hans_Bethe.
External links
Source attribution: Biography:Hans Bethe