SciTech Connect

Title: TEMPERATURE AND DENSITY CONDITIONS FOR NUCLEOGENESIS BY FUSION PROCESSES IN STARS

TEMPERATURE AND DENSITY CONDITIONS FOR NUCLEOGENESIS BY FUSION PROCESSES IN STARS 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.)
Authors:
Publication Date:
OSTI Identifier:OSTI ID: 4308210
Report Number(s):A/CONF.15/P/353
Resource Type:Technical Report
Resource Relation:Other Information: Prepared for the Second U.N. International Conference on the Peaceful Uses of Atomic Energy, 1958. Orig. Receipt Date: 31-DEC-58
Research Org:California Inst. of Tech., Pasadena. W.K. Kellogg Lab. of Radiation
Sponsoring Org:US Atomic Energy Commission (AEC)
Country of Publication:United States
Language:English
Subject: PHYSICS; ASTROPHYSICS; COSMOLOGY; DENSITY; ELEMENTS; NUCLEI; PRODUCTION; QUANTITY RATIO; STARS; TEMPERATURE; THERMONUCLEAR REACTIONS Stars-Thermonuclear Reactions