Ground states of nuclei and neutron stars
β Scribed by V.R. Pandharipande
- Publisher
- Elsevier Science
- Year
- 1993
- Tongue
- English
- Weight
- 947 KB
- Volume
- 553
- Category
- Article
- ISSN
- 0375-9474
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The role of the equation of state in the structure of neutron stars is summarized. At densities beyond a few times the normal nuclear saturation density, the neutron-proton-electron sea can be supplemented with more exotic matter, usually involving strangeness, such as hyperons, kaon or pion condens
Alpha half lives, branching ratios and hindrance factors of even-even nuclei in the range 78 Z 102 from ground state to ground state and ground state to excited states of daughter nuclei are computed using the Coulomb and proximity potential model for deformed nuclei (CPPMDN). The computed half life