Speaker
Harish Chandra Das
(Institute of Physics, Bhubaneswar)
Description
It is the most common assumption is that the pressure inside the neutron star (NS) is isotropic in nature. In this study, we calculate the anisotropic pressure inside the NS and calculate its effects on some properties such as mass, radius, compactness, and surface curvature. To obtain the NS properties, we use the relativistic mean-field equation of states. We observed that anisotropy has significant effects on the surface curvature of the NS.
| Session | Astroparticle Physics and Cosmology |
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Author
Harish Chandra Das
(Institute of Physics, Bhubaneswar)
Co-authors
Mr
Ankit Kumar
(Institute of Physics, Bhubaneswar)
Mr
Vishal Parmar
(School of Physics and Materials Science, Thapar Institute of Engineering and Technology, Patiala 147004, India)
Prof.
Suresh Kumar Patra
(Institute of Physics, Bhubaneswar)
