Towards the Equation of State for Dense Stellar Matter
Küçük Resim Yok
Tarih
2010
Dergi Başlığı
Dergi ISSN
Cilt Başlığı
Yayıncı
IOP PUBLISHING LTD
Erişim Hakkı
info:eu-repo/semantics/openAccess
Özet
The thermal nuclear multifragmentation reaction can be used to investigate the nuclear liquid-gas phase coexistence region and its relation to the astrophysical processes such as the collapse of massive stars, and the supernova type-II explosions. We have performed some calculations to estimate stellar equation of state (EOS) on the basis of statistical multifragmentation model.
Açıklama
4th International Conference on Nuclear Physics in Astrophysics -- JUN 08-12, 2009 -- Lab Nazl Frascati, Frascati, ITALY
Anahtar Kelimeler
Kaynak
NUCLEAR PHYSICS IN ASTROPHYSICS IV (NPAIV 2009)
WoS Q Değeri
N/A
Scopus Q Değeri
N/A
Cilt
202
