112 citations · 754 across the 30 of their papers we have counts for
29 papers
Dark Matter Influence on Quarkyonic Stars: A Relativistic Mean Field Analysis
D. Dey, Jeet Amrit Pattnaik, H. C. Das +3
The formulation of quarkyonic matter consists of treating both quarks and nucleons as quasi-particles, where a cross-over transition occurs between the two phases. This work is bas…
Constraining neutron star properties and dark matter admixture with the NITR-I equation of state: Insights from observations and universal relations
Pinku Routaray, H C Das, Jeet Amrit Pattnaik +1
A recent observational study has constrained the maximum mass of neutron stars (NSs), with particular attention to PSR J0952-0607 and the compact star remnant HESS J1731-347, espec…
Influence of Dark Matter on the Magnetized Neutron Star
Vishal Parmar, H. C. Das, M. K. Sharma +1
Over the past two decades, significant strides have been made in the study of Dark Matter (DM) admixed neutron stars and their associated properties. However, an intriguing facet r…
Anisotropic Strange Stars in the Spotlight: Unveiling Constraints through Observational Data
H. C. Das, Luiz L. Lopes
Motivated by the recent suggestions that very massive pulsar (PSR J0952-0607) and very light compact object (HESS J1731-347) exist, in this article, we revisit the possibility of s…
Impacts of dark matter interaction on nuclear and neutron star matter within the relativistic mean-field model
H. C. Das
This thesis explores the effects of dark matter (DM) on neutron stars (NSs) using the relativistic mean-field (RMF) model. The effects of DM on NS properties, including the mass-ra…
The Impact of Anisotropy on Neutron Star Properties: Insights from I-f-C Universal Relations
Sailesh Ranjan Mohanty, Sayantan Ghosh, Pinku Routaray +2
This study presents a universal relation for anisotropic neutron stars, called the relation, which accounts for the local anisotropic pressure using the Quasi-Local (QL) Mo…
Constraining the Surface Curvature of an Anisotropic Neutron Star
H. C. Das, Jeet Amrit Pattnaik, S. K. Patra
The anisotropy of pressure arises due to the various complex phenomena that happen inside the neutron star (NS). In this study, we calculate the degree of anisotropy inside the NS…
Radial Oscillations of Dark Matter admixed Neutron Stars
Pinku Routray, H. C. Das, Souhardya Sen +3
Within the relativistic mean-field model, we investigate the properties of dark matter (DM) admixed neutron stars, considering non-rotating objects made of isotropic matter. We ado…
Magnetised neutron star crust within effective relativistic mean-field model
Vishal Parmar, H. C. Das, M. K. Sharma +1
Even though the crystallize nature of the neutron star crust plays a pivotal role in describing various fascinating astrophysical observations, its microscopic structure is not ful…
Love relation for an anisotropic neutron star
H. C. Das
One of the most common assumptions has been made that the pressure inside the star is isotropic in nature. However, the pressure is locally anisotropic in nature which is a more re…
Pasta properties of the neutron star within effective relativistic mean-field model
Vishal Parmar, H. C. Das, Ankit Kumar +3
We study the properties of pasta structures and their influence on the neutron star observables employing the effective relativistic mean-field (E-RMF) model. The compressible liqu…
Thermal Relaxation of Dark Matter Admixed Neutron Star
Ankit Kumar, H. C. Das, S. K. Patra
Motivated by the various theoretical studies regarding the efficient capturing of dark matter by neutron stars, we explore the possible indirect effects of captured dark matter on…
Dark Matter Effects on the Compact Star Properties
H. C. Das, Ankit Kumar, Bharat Kumar +1
The neutron star properties are generally determined by the equation of state of -equilibrated dense matter. In this work, we consider the interaction of fermionic dark matter (…
Systematic study for the surface properties of neutron star
Ankit Kumar, H. C. Das, Jeet Amrit Pattnaik +1
[Background] In our earlier work {\bf [Phys. Rev. C 104, 055804 (2021)]}, we studied the surface properties of a neutron star, assuming it as a huge finite nucleus containing proto…
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…
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…
Thermal impacts on the properties of nuclear matter and young neutron star
Ankit Kumar, H. C. Das, M. Bhuyan +1
We present a methodical study of the thermal and nuclear properties for the hot nuclear matter using relativistic-mean field theory. We examine the effects of temperature on the bi…
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…
Correlation between the curvature and some properties of the neutron star
S. K. Biswal, H. C. Das, Ankit Kumar +4
According to the general theory of relativity, a massive body induces curvature in the surrounding spacetime. In this study, the surface curvature (SC) of neutron stars is computed…
BigApple force and its implications to finite nuclei and astrophysical objects
H. C. Das, Ankit Kumar, Bharat Kumar +2
The secondary component of the GW190814 event left us with a question, "whether it is a supermassive neutron star or lightest black-hole?". Recently, Fattoyev et al. have obtained…