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Impact of nuclear mass models on $r$-process nucleosynthesis and heavy element abundances in $r$-process enhanced metal-poor stars

Fuente: arXiv

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Dettagli Bibliografici
Autori principali:	Chen, Meng-Hua, Li, Li-Xin, Liang, En-Wei, Wang, Ning
Natura:	Preprint
Pubblicazione:	2024
Soggetti:	High Energy Astrophysical Phenomena Solar and Stellar Astrophysics Nuclear Theory
Accesso online:	Acceder al recurso
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