1. Rates of Nuclear Reactions in White-Dwarf Stars. 2. The Cooling of Neutron Stars
<p>1. Rates of Nuclear Reactions in White-Dwarf Stars</p> <p>In stellar matter as cool and dense as the interior of a white dwarf, the Coulomb energies between neighboring nuclei are large compared to the kinetic energies of the nuclei. Each nucleus is constrained to vibrate abo...
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| Format: | Others |
| Language: | en |
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1966
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| Online Access: | https://thesis.library.caltech.edu/3714/3/wolf-ra_1966.pdf Wolf, Richard Alan (1966) 1. Rates of Nuclear Reactions in White-Dwarf Stars. 2. The Cooling of Neutron Stars. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/FKB7-W110. https://resolver.caltech.edu/CaltechETD:etd-09232002-145100 <https://resolver.caltech.edu/CaltechETD:etd-09232002-145100> |
Internet
https://thesis.library.caltech.edu/3714/3/wolf-ra_1966.pdfWolf, Richard Alan (1966) 1. Rates of Nuclear Reactions in White-Dwarf Stars. 2. The Cooling of Neutron Stars. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/FKB7-W110. https://resolver.caltech.edu/CaltechETD:etd-09232002-145100 <https://resolver.caltech.edu/CaltechETD:etd-09232002-145100>