11 pp.
11 pp.
| 1330 K 11 pp. | |
| View Document | ||
| Title | Temperature and Density Conditions for Nucleogenesis by Fusion Processes in Stars | |
| Author(s) | Fowler, W. A. | |
| Publication Date | June 1958 | |
| Report Number | A/CONF.15/P/353 | |
| Unique Identifier | ACC0134 | |
| Other Numbers | OSTI ID: 4308210 | |
| Research Org | W. K. Kellogg Radiation Laboratory, California Inst. of Tech., Pasadena, CA | |
| Sponsoring Org | US Atomic Energy Commission (AEC) | |
| Other Information | Prepared for the Second U.N. International Conference on the Peaceful Uses of Atomic Energy, 1958 | |
| Subject | Physics; Astrophysics; Cosmology; Density; Elements; Nuclei; Production; Quantity Ratio; Stars; Temperature; Thermonuclear Reactions | |
| Keywords | Stars - Thermonuclear Reactions | |
| Related Web Pages | William Fowler and Elements in the Stars | |
| Abstract | 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.) | |
| 1330 K 11 pp. | |
| View Document | ||
