Nuclear Astrophysics
Copyright policy )Nuclear Astrophysics
The problem of core-collapse supernovae is used to illustrate the many connections between nuclear astrophysics and the problems nuclear physicists study in terrestrial laboratories. Efforts to better understand the collapse and mantle ejection are also motivated by a variety of interdisciplinary issues in nuclear, particle, and astrophysics, including galactic chemical evolution, neutrino masses and mixing, and stellar cooling by the emission of new particles. The current status of theory and observations is summarized.
- University of North Texas United States
- University of Mary United States
- Washington State University United States
- University of Washington United States
General Physics, Beta Decay 663400, Star Evolution, 73 Nuclear Physics And Radiation Physics, Eruptive Variable Stars, Variable Stars 663400* -- Specific Nuclear Reactions & Scattering-- (1992-), Synthesis, R Process, 661300 -- Other Aspects Of Physical Science-- (1992-), Nuclear Reactions, Neutrino Reactions, Other Aspects Of Physical Science, Mathematical Models, 661300, Decay, Beta Decay, Specific Nuclear Reactions And Scattering, Stars, Supernovae, Shock Waves, Lepton Reactions, 71 Classical And Quantum Mechanics, Nucleosynthesis, Nuclear Decay
General Physics, Beta Decay 663400, Star Evolution, 73 Nuclear Physics And Radiation Physics, Eruptive Variable Stars, Variable Stars 663400* -- Specific Nuclear Reactions & Scattering-- (1992-), Synthesis, R Process, 661300 -- Other Aspects Of Physical Science-- (1992-), Nuclear Reactions, Neutrino Reactions, Other Aspects Of Physical Science, Mathematical Models, 661300, Decay, Beta Decay, Specific Nuclear Reactions And Scattering, Stars, Supernovae, Shock Waves, Lepton Reactions, 71 Classical And Quantum Mechanics, Nucleosynthesis, Nuclear Decay
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