22 citations · 79 across the 8 of their papers we have counts for
8 papers
Exploration of Nuclear Matter Properties and Related Thermodynamical Aspects
Vishal Parmar
In this study, my main goal is to examine the nuclear matter properties across a wide range of conditions, such as temperature, density, asymmetry, pressure, and magnetic field. Un…
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…
Critical Properties of Symmetric Nuclear Matter in Low-Density Regime Using Effective-Relativistic Mean Field Formalism
Vishal Parmar, Manoj K Sharma, S K Patra
The effective field theory motivated relativistic mean-field (E-RMF) formalism is employed to study the equation of state (EoS) for the infinite symmetric nuclear matter at finite…
Thermal effects in hot and dilute homogeneous asymmetric nuclear matter
Vishal Parmar, Manoj K Sharma, S K Patra
We present a comprehensive analysis of hot and dilute isospin-asymmetric nuclear matter employing the temperature-dependent effective-relativistic mean-field theory (E-RMF). The E-…
Properties of hot finite nuclei and associated correlations with infinite nuclear matter
Vishal Parmar, Manoj K Sharma, S K Patra
This work aim to study the various thermal characteristics of nuclei in view of the saturation and critical behavior of infinite nuclear matter. The free energy of a nucleus is par…
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…
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…
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…