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TEMPERATURE AND DENSITY CONDITIONS FOR NUCLEOGENESIS BY FUSION PROCESSES IN STARS

Technical Report ·
DOI:https://doi.org/10.2172/4308210· OSTI ID:4308210

An attempt is made to correlate nuclear findings with what is known about stellar evolution. Some discussion is given to present research in nuclear physics and astrophysics which may lead to further elucidation of the problem of nucleogenesis and of its cosmological implications. (M.H.R.)

Research Organization:
California Inst. of Tech., Pasadena. W.K. Kellogg Lab. of Radiation
Sponsoring Organization:
US Atomic Energy Commission (AEC)
NSA Number:
NSA-12-014843
OSTI ID:
4308210
Report Number(s):
A/CONF.15/P/353
Country of Publication:
United States
Language:
English

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