Constraining Tidal deformability from finite nuclei data, Bijay Agrawal (Saha Institute of Nuclear Physics)

*Please note that this seminar will take place at 11:00am ET

Bijay Agrawal

Saha Institute of Nuclear Physics

The tidal deformability inferred from the Gravitational Waves, which are emitted by merging neutron stars, are instrumental in determining the equation of state (EoS) of dense matter. The importance of the observed finite nuclei properties in unveiling the correlations of the tidal deformability with the key EoS parameters will be discussed. Further, it will be shown that suitably chosen experimental data on isoscalar and isovector sensitive nuclear observables complemented with the observed maximum neutron star mass can impose tighter constrains on tidal deformability