TEMPERATURE AND DENSITY CONDITIONS FOR NUCLEOGENESIS BY FUSION PROCESSES IN STARS

Technical Report · Sun Jun 01 00:00:00 EDT 1958

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

Fowler, W A

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
• 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
• Country of Publication: United States
• Language: English

Related Subjects

PHYSICS
ASTROPHYSICS
COSMOLOGY
DENSITY
ELEMENTS
NUCLEI
PRODUCTION
QUANTITY RATIO
STARS
TEMPERATURE
THERMONUCLEAR REACTIONS
Stars-Thermonuclear Reactions