Speaker
Bijay Kumar Agrawal
(Saha Institute of Nuclear Physics)
Description
The impacts of various symmetry energy parameters on the properties of neutron stars have been recently investigated, and the outcomes are at variance. Results obtained from systematic analysis of the correlations of slope and curvature parameters of symmetry energy at the saturation density with the tidal deformability and stellar radius of non-spinning neutron stars in the mass range of 1.2–1.6M⊙ will be discussed.
Primary authors
Bijay Kumar Agrawal
(Saha Institute of Nuclear Physics)
Mr
N Patra
(BITS -Pilani Goa Campus)
Mr
A Venneti
(BITS-Pilani Hyderabad )
Mr
SK. Adil Imam
Prof.
A Mukherjee