Stiffening baryonic equation of state with hyperons

نویسندگانM. Ghazanfari Mojarrad
همایشThe Modern Physics of Compact Stars and Relativistic Gravity
تاریخ برگزاری همایش2015
نوع ارائهسخنرانی
سطح همایشبین المللی

چکیده مقاله

Study of the structure and properties of neutron stars (NS) has attracted ever increasing theoretical and observational efforts during the last few decades [1]. The baryonic equation of state (EOS) is an essential step towards creating an efficient and convenient model for NS structure and composition [2-4]. Recent observations of two solar-mass NS, lead the EOS of theoretical models to a more stiff behavior until a value greater than of this value for the maximum mass of NS is obtained.