TABULATED EQUATION OF STATE FOR SUPERNOVA MATTER INCLUDING FULL NUCLEAR ENSEMBLE
Küçük Resim Yok
Tarih
2014
Dergi Başlığı
Dergi ISSN
Cilt Başlığı
Yayıncı
IOP PUBLISHING LTD
Erişim Hakkı
info:eu-repo/semantics/openAccess
Özet
This is an introduction to the tabulated database of stellar matter properties calculated within the framework of the Statistical Model for Supernova Matter (SMSM). The tables present thermodynamical characteristics and nuclear abundances for 31 values of baryon density (10(-8) < rho/rho(0) < 0.32, rho(0) = 0.15 fm(-3) is the normal nuclear matter density), 35 values of temperature (0.2MeV < T < 25 MeV), and 28 values of electron-to-baryon ratio (0.02 < Y-e < 0.56). The properties of stellar matter in beta equilibrium are also considered. The main ingredients of the SMSM are briefly outlined, and the data structure and content of the tables are explained.
Açıklama
Anahtar Kelimeler
dense matter, equation of state, nuclear reactions, nucleosynthesis, abundances, stars: neutron, supernovae: general
Kaynak
ASTROPHYSICAL JOURNAL
WoS Q Değeri
Q1
Scopus Q Değeri
Q1
Cilt
789
Sayı
1
