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pro vyhledávání: '"Hamsa S. Jasim"'
Publikováno v:
IOSR Journal of Applied Physics. :43-52
Nuclear state density was calculated for the nuclear reaction inside the core of three different main- sequence stars namely, Sun, Sirius and Vega. The selected nuclei for present calculation were H 4 , C 12 , N 14 , and O 16 ; and the state density
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7b68b3332dc038eca4b88b2caf4be2b6
https://doi.org/10.9790/4861-0804014352
https://doi.org/10.9790/4861-0804014352
