Scopus
🔓 Açık Erişim YÖKSİS Eşleşti
Tabulated equation of state for supernova matter including full nuclear ensemble
Astrophysical Journal · Temmuz 2014
YÖKSİS Kayıtları
Tabulated Equation of State for Supernova MAtter Including Full Ensemble
ASTROPHYSICAL JOURNAL · 2014 SCI-Expanded 3 atıf
PROFESÖR NİHAL BÜYÜKÇİZMECİ →
Makale Bilgileri
DergiAstrophysical Journal
Yayın TarihiTemmuz 2014
Cilt / Sayfa789
Scopus ID2-s2.0-84902578919
Erişim🔓 Açık Erişim
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 < ρ/ρ0 < 0.32, ρ0 = 0.15 fm-3 is the normal nuclear matter density), 35 values of temperature (0.2 MeV < T < 25 MeV), and 28 values of electron-to-baryon ratio (0.02 < Ye < 0.56). The properties of stellar matter in β equilibrium are also considered. The main ingredients of the SMSM are briefly outlined, and the data structure and content of the tables are explained. © 2014. The American Astronomical Society. All rights reserved.
Yazarlar (3)
1
Nihal Buyukcizmeci
2
A. S. Botvina
3
I. N. Mishustin
Anahtar Kelimeler
dense matter
equation of state
nuclear reactions, nucleosynthesis, abundances
stars: neutron
supernovae: general
Kurumlar
Frankfurt Institute for Advanced Studies
Frankfurt am Main Germany
Institute for Nuclear Research of the Russian Academy of Sciences
Moscow Russian Federation
Johannes Gutenberg-Universität Mainz
Mainz Germany
National Research Centre "Kurchatov Institute"
Moscow Russian Federation
Selçuk Üniversitesi
Selçuklu Turkey
Metrikler
28
Atıf
3
Yazar
5
Anahtar Kelime