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pro vyhledávání: '"Marcelo Gimenez Munhoz"'
Autor:
R. G. Pizzone, I. Indelicato, Marisa Gulino, G. L. Guardo, Silvio Cherubini, Giuseppe D’Agata, Ivano Lombardo, Roberto Menegazzo, Claudio Spitaleri, Antonio Caciolli, S. M. R. Puglia, Maria Letizia Sergi, Marcelo Gimenez Munhoz, Marco La Cognata, Carlo Broggini, Nelson Carlin, Rosanna Depalo, V. Rigato, Daniele Dell’Aquila, Alexandra Cvetinovic, Stefano Romano, Salvo Tudisco, Aurora Tumino, F. A. Souza, Roberta Spartà, Livio Lamia, G. G. Rapisarda
Publikováno v:
EPJ Web of Conferences, Vol 165, p 01042 (2017)
The 10 B(p,α )7 Be reaction is the main responsible for the 10 B destruction in stellar interior [1]. In such environments this p-capture process occurs at a Gamow energy of 10 keV and takes places mainly through a resonant state (Ex = 8.701 MeV) of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6805fa80fbb45dba4acb130327119ac6
https://doaj.org/article/ce191a1694f34197b0c3a2d71dec6277
https://doaj.org/article/ce191a1694f34197b0c3a2d71dec6277
