Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/9180
Title: Supernova matter: a semiclassical approach
Author: Pi Pericay, Martí
Viñas Gausí, Xavier
Barranco Gómez, Manuel
Polls Martí, Artur
Pérez-Canyellas, A.
Keywords: Evolució estel·lar
Astrofísica
Equacions d'estat
Stellar evolution
Astrophysics
Equation of state
Issue Date: 1986
Publisher: EDP Sciences
Abstract: A well-established semiclassical method is used to systematically study the properties of hot dense matter in the conditions prevailing during the gravitational collapse of massive stars. Different semiclassical kinetic energy and entropy densities are discussed. Detailed results for different nuclear forces having different nucleon effective mass and nuclear incompressibility are presented. Plasma effects (translational and vibrational energies and Coulomb excess) are considered for a typical adiabat. The results presented here cover a wide range in entropy per baryon and electron concentration per baryon, for baryon densities ranging from 0.001/cu fm to 0.3/cu fm.
Note: Reproducció digital del document publicat en format paper, proporcionada per NASA Astrophysics Data System http://adsabs.harvard.edu/full/1986A%26AS...64..439P
It is part of: Astronomy and Astrophysics Supplement Series, 1986, vol. 64, núm. 3, p. 439-451.
URI: http://hdl.handle.net/2445/9180
ISSN: 0365-0138
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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