| نویسندگان | M. Ghazanfari Mojarrad |
|---|---|
| همایش | The Modern Physics of Compact Stars and Relativistic Gravity |
| تاریخ برگزاری همایش | 2015 |
| نوع ارائه | سخنرانی |
| سطح همایش | بین 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.