267 citations · 1k across the 33 of their papers we have counts for
8 papers · 1 filter
Crustal properties of a neutron star within an effective relativistic mean-field model
Vishal Parmar, H. C. Das, Ankit Kumar +2
We use the effective relativistic mean-field (E-RMF) model to study the crustal properties of the neutron star. The unified equations of state (EoS) are constructed using recently…
Constraining nuclear matter parameters and neutron star observables using PREX-2 and NICER data
S. K. Biswal, H. C. Das, Ankit Kumar +1
We try to constraints some of the nuclear matter parameters such as symmetry energy () and its slope () from the recent inferred data of the PREX-2. Other nuclear matter para…
Dark matter admixed neutron star as a possible compact component in the GW190814 merger event
H. C. Das, Ankit Kumar, S. K. Patra
We put constraints on the secondary component of GW190814 by analyzing the observational data of the event. The relativistic mean-field models are used to calculate the mass-radius…
Impacts of dark matter on the -mode oscillation of hyperon star
H. C. Das, Ankit Kumar, S. K. Biswal +1
We investigate the -mode oscillation of the dark matter admixed hyperon star within the relativistic Cowling approximation. The macroscopic properties are calculated with the re…
Incompressibility and Symmetry Energy of Neutron Star
Ankit Kumar, H. C. Das, S. K. Patra
We trace a systematic and consistent method to precisely numerate the magnitude range for various structural and isospin compositional properties of the neutron star. Incompressibi…
Heavy Magnetic Neutron Stars
I. A. Rather, Usuf Rahaman, V. Dexheimer +2
We systematically study the properties of pure nucleonic and hyperonic magnetic stars using a density-dependent relativistic mean field (DD-RMF) equations of state. We explore seve…
Effects of dark matter on the in-spiral properties of the binary neutron stars
H. C. Das, Ankit Kumar, S. K. Patra
Using the relativistic mean-field model, we calculate the properties of binary neutron star (BNS) in the in-spiral phase. Assuming the dark matter (DM) particles are accreted insid…
Rotating neutron stars with quark cores
I. A. Rather, Usuf Rahaman, M. Imran +3
The rotating neutron star properties are studied with a phase transition to quark matter. The density-dependent relativistic mean-field model (DD-RMF) is employed to study the hadr…