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  1. en.wikipedia.org › wiki › Hans_BetheHans Bethe - Wikipedia

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

  2. 28 de jun. de 2024 · Hans Bethe was a German-born American theoretical physicist who helped shape quantum physics and increased the understanding of the atomic processes responsible for the properties of matter and of the forces governing the structures of atomic nuclei. He received the Nobel Prize for Physics in 1967.

  3. 26 de jun. de 2024 · In the late 1930s Hans Bethe first recognized that the fusion of hydrogen nuclei to form deuterium is exoergic (i.e., there is a net release of energy) and, together with subsequent nuclear reactions, leads to the synthesis of helium.

  4. 26 de jun. de 2024 · The German-born physicist Hans Bethe proposed in the 1930s that the H-H fusion reaction could occur with a net release of energy and provide, along with subsequent reactions, the fundamental energy source sustaining the stars.

  5. Hace 5 días · At Los Alamos, Feynman was assigned to Hans Bethe's Theoretical (T) Division, and impressed Bethe enough to be made a group leader. He and Bethe developed the Bethe–Feynman formula for calculating the yield of a fission bomb, which built upon previous work by Robert Serber. As a junior physicist, he was not central to the project.

  6. Hace 4 días · A theory verified by Hans Bethe in 1939 showed that beta decay and quantum tunneling in the Sun's core might convert one of the protons into a neutron and thereby produce deuterium rather than a diproton. The deuterium would then fuse through other reactions to further increase the energy output.

  7. Hace 6 días · the cross section of the interaction has been provided by Hans Bethe and W alter Heitler. in 1934 [1], it was not until the disco very of the cosmic-wav e background radiation in the. mid-sixties [2

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