activity
20202025
most citedEffect of Dark matter and -cut potential on radial and non-radial oscillation modes in neutron stars

4 citations · 4 across the 3 of their papers we have counts for

collaborators
Showing nucl-thShow all

7 papers · 1 filter

nucl-th2025

Radial and Non-Radial Oscillations of Protoneutron Stars with Hyperonic Composition

Prashant Thakur, Adamu Issifu, Ishfaq Ahmad Rather +2

This paper explores radial and non-radial oscillations of protoneutron stars (PNSs) as they evolve from hot, neutrino-rich configurations through deleptonization to cold, catalyzed…

nucl-th2024

Radial Oscillations in Hybrid Stars with Slow Quark Phase Transition

Ishfaq Ahmad Rather, Kauan D. Marquez, Betânia C. Backes +2

This study investigates the radial oscillations of hybrid neutron stars, characterized by a composition of hadronic external layers and a quark matter core. Utilizing a density-dep…

nucl-th2021

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…

nucl-th2021

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…

nucl-th2020

Hadron-Quark phase transition in the context of GW190814

I. A. Rather, A. A. Usmani, S. K. Patra

The properties of the neutron stars are calculated for the hadronic matter within the density-dependent relativistic mean-field model (DD-RMF). The phase transition to the quark ma…

nucl-th2020

Effect of Inner Crust EoS on Neutron star properties

Ishfaq Ahmad Rather, Anisul Ain Usmani, Suresh Kumar Patra

The neutron star maximum mass and the radius are investigated within the framework of the relativistic mean-field (RMF) model. The variation in the radius at the canonical mass, $R…