Thermonuclear 28P(p, γ)29S reaction rate and astrophysical implication in ONe nova explosion

[Context] An accurate 28P(p, γ)29S reaction rate is crucial to defining the nucleosynthesis products of explosive hydrogen burning in ONe novae. Using the recently released nuclear mass of 29S, together with a shell model and a direct capture calculation, we reanalyzed the 28P(p, γ)29S thermonuclear...

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Detalles Bibliográficos
Autores: Liu, J. B., Ramasco, José J., Hou, S. Q., Pignatari, M., Trueman, T. C.L., Longland, R., Li, J. G., Bertulani, C. A., Xu, X. X.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2024
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/383268
Acceso en línea:http://hdl.handle.net/10261/383268
https://api.elsevier.com/content/abstract/scopus_id/85200537943
Access Level:acceso abierto
Palabra clave:Novae, cataclysmic variables
Nuclear reactions, nucleosynthesis, abundances
Stars: abundances
Descripción
Sumario:[Context] An accurate 28P(p, γ)29S reaction rate is crucial to defining the nucleosynthesis products of explosive hydrogen burning in ONe novae. Using the recently released nuclear mass of 29S, together with a shell model and a direct capture calculation, we reanalyzed the 28P(p, γ)29S thermonuclear reaction rate and its astrophysical implication.

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