activity
20172026
most citedGW170817: constraining the nuclear matter equation of state from the neutron star tidal deformability

267 citations · 919 across the 56 of their papers we have counts for

collaborators
Showing 2020Show all

5 papers · 1 filter

astro-ph.HE2020★ 14 cited

New equation of state involving Bose-Einstein condensate of antikaon for supernova and neutron star merger simulations

Tuhin Malik, Sarmistha Banik, Debades Bandyopadhyay

We compute a new equation of state table including Bose-Einstein condensate of mesons for core collapse supernova and neutron star merger simulations. Nuclei and interactin…

nucl-th2020★ 3 cited

Dark matter admixed neutron star properties in the light of gravitational wave observations: a two fluid approach

Arpan Das, Tuhin Malik, Alekha C. Nayak

We consider the effect of density dependent dark matter on the neutron star mass, radius, and tidal deformability. Nuclear matter (normal matter) as well as the fermionic dark matt…

nucl-th2020★ 25 cited

Unveiling the correlations of tidal deformability with the nuclear symmetry energy parameters

Tuhin Malik, B. K. Agrawal, Constança Providência +1

The chi-squared based covariance approach allows one to estimate the correlations among desired observables related to nuclear matter directly from a set of fit data without taking…

nucl-th2020★ 16 cited

Constraining nuclear matter parameters from correlation systematics:a mean-field perspective

B. K. Agrawal, Tuhin Malik, J. N. De +1

The nuclear matter parameters define the nuclear equation of state (EoS), they appear as coefficients of expansion around the saturation density of symmetric and asymmetric nuclear…

physics.comp-ph2020★ 16 cited

The Neutron Star Outer Crust Equation of State: A Machine Learning approach

Murarka Utsav Anil, Kinjal Banerjee, Tuhin Malik +1

Constructing the outer crust of the neutron stars requires the knowledge of the Binding Energy (BE) of the atomic nuclei. Although the BE of a lot of the nuclei is experimentally d…