The 180Ta production puzzle and the classical s-process

Autor:	P. Alexa, M. Wuerkner, Jorrit de Boer, M. Loewe
Rok vydání:	2003
Předmět:	Physics Nuclear and High Energy Physics Stellar nucleosynthesis Abundance (ecology) Astrophysics::High Energy Astrophysical Phenomena Astrophysics::Solar and Stellar Astrophysics Production (computer science) Astrophysics s-process Astrophysics::Galaxy Astrophysics
Zdroj:	Nuclear Physics A. 719:C275-C278
ISSN:	0375-9474
Popis:	The production and survival of the quasistable isomer $^{180}$Ta during the stellar nucleosynthesis has remained a matter of discussion for years. A careful analysis of the available experimental data and theoretical calculations enabled us to reproduce the observed solar abundance of $^{180}$Ta in the classical s-process ($kT=28$ keV -- 33 keV).
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_________::e3a4889099688e44756d62a0a6a5e4ab https://doi.org/10.1016/s0375-9474(03)00931-x Zobrazit plný text záznamu Full Text from ScienceDirect