Revisiting the 3α reaction rates in helium burning stars
Helium burning is one of the most fundamental steps of stellar nucleosynthesis, as it describes the formation of life-determining element of carbon, while it plays a key role in the evolution of Red Giant, accreting White Dwarfs and Neutron Stars. In this work we develop a generalized statistical th...
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Main Authors: | T. Depastas, S.T. Sun, H.B. He, H. Zheng, A. Bonasera |
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Format: | Article |
Language: | English |
Published: |
Elsevier
2025-01-01
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Series: | Physics Letters B |
Subjects: | |
Online Access: | http://www.sciencedirect.com/science/article/pii/S037026932400738X |
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