From the Sun to supernovae: experimental determinations of stellar reaction rates at TRIUMF
作者： Jennifer Fallis
DOI: 10.1088/1742-6596/420/1/012148
关键词: Supernova 、 Asymptotic giant branch 、 Resonance (particle physics) 、 Astrophysics 、 Stars 、 Reaction rate 、 Nuclear physics 、 Physics 、 Solar neutrino 、 Nucleosynthesis
摘要: The ongoing goal of the TRIUMF astrophysics group is to measure resonance strengths and cross sections for reactions astrophysical importance. This done using accelerated radioactive stable beams from ISAC I II delivered DRAGON TUDA facilities. wide range available at energies provided by accelerators enable us reaction rates interest in many different environments. Experiments past year have studied important understanding production solar neutrinos as well nucleosynthesis Big Bang, Asymptotic Giant Branch (AGB) stars, novae, supernovae. These experiments various techniques required these measurements will be discussed.
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