| Authors | M. Ghazanfari Mojarrad |
|---|---|
| Conference Title | The Modern Physics of Compact Stars and Relativistic Gravity |
| Holding Date of Conference | 2015 |
| Presentation | SPEECH |
| Conference Level | International Conferences |
Abstract
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.