Nuclear equation of state and the structure of neutron stars
Jazyk: | angličtina |
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Rok vydání: | 2006 |
Předmět: | |
Zdroj: | SUPERDENSE QCD MATTER AND COMPACT STARS. :93-111 |
ISSN: | 1568-2609 |
Popis: | The hadronic equation of state for a neutron star is discussed with a particular emphasis on the symmetry energy. The results of several microscopic approaches are compared and also a new calculation in terms of the self-consistent Green function method is presented. In addition possible constraints on the symmetry energy coming from empirical information on the neutron skin of finite nuclei are considered. |
Databáze: | OpenAIRE |
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