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The r-, s-, and p-processes in nucleosynthesis
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Meyer, Bradley S. |
| Copyright Year | 1994 |
| Description | A goal of this paper is to review the recent progress astrophysicists, astronomers, and physicists have made in the r-, s-, and p-processes in nucleosynthesis and to point out the problems that remain in our understanding of the formation of the heavy nuclei. Another, perhaps deeper, goal is to to seek some understanding of why there are three major processes available to nature for synthesis of heavy elements. |
| File Size | 1819238 |
| Page Count | 38 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19980007188 |
| Archival Resource Key | ark:/13960/t9z082b5q |
| Language | English |
| Publisher Date | 1994-01-01 |
| Access Restriction | Open |
| Subject Keyword | Atomic And Molecular Physics Stellar Winds Heavy Elements Neutron Stars Astrophysics Nuclear Fusion Supernovae Heavy Nuclei Abundance Entropy Asymptotic Giant Branch Stars Equilibrium Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
