267 citations · 456 across the 11 of their papers we have counts for
11 papers
Estimating nuclear equation of state parameters away from saturation density
Naosad Alam, Subrata Pal
We explore the density variation of the correlation coefficient of the key parameters of the nuclear equation of state (EoS) with the bulk and crustal properties of neutron stars.…
Impact of modified gravity theory on neutron star and nuclear matter properties
Naosad Alam, Subrata Pal, A. Rahmansyah +1
New observational data, measured with a high degree of accuracy, of compact isolated neutron stars and binary stars in gravitational wave remnants have the potential to explore the…
A Detailed Analysis of the Special Points on Solutions of Hybrid (Twin) Stars
Debashree Sen, Naosad Alam, Gargi Chaudhuri
Hadron-quark phase transition in neutron star cores is achieved in the present work with the help of Maxwell construction. For the purpose we employ six different and well-known ha…
Estimation of transport coefficients of dense hadronic and quark matter
Debashree Sen, Naosad Alam, Sabyasachi Ghosh
We calculate the transport coefficients like shear viscosity and electrical conductivity with respect to density of dense hadronic and quark matter. By considering the simple massl…
Properties of Hybrid Stars with Density Dependent Bag Model
Debashree Sen, Naosad Alam, Gargi Chaudhuri
The phenomena of deconfinement of hadronic matter into quark matter at high density, relevant to hybrid star (HS) cores, is studied in the present work. The effective chiral model…
GW170817: constraining the nuclear matter equation of state from the neutron star tidal deformability
Tuhin Malik, N. Alam, M. Fortin +5
Constraints set on key parameters of the nuclear matter equation of state (EoS) by the values of the tidal deformability, inferred from GW170817, are examined by using a diverse se…
Warm unstable asymmetric nuclear matter: critical properties and the density dependence of the symmetry energy
N. Alam, H. Pais, C. Providência +1
The spinodal instabilities in hot asymmetric nuclear matter and some important critical parameters derived thereof are studied using six different families of relativistic mean-fie…
Strong correlations of neutron star radii with the slopes of nuclear matter incompressibility and symmetry energy at saturation
N. Alam, B. K. Agrawal, M. Fortin +4
We examine the correlations of neutron star radii with the nuclear matter incompressibility, symmetry energy, and their slopes, which are the key parameters of the equation of stat…
Diversities in the properties of neutron stars at a fixed neutron-skin thickness in Pb nucleus
N. Alam, A. Sulaksono, B. K. Agrawal
We study the diversities in the properties of the neutron stars arising due to the different choices for the cross-coupling between various mesons which governs the density depende…
Core-crust transition properties of neutron stars within systematically varied extended relativistic mean-field model
A. Sulaksono, Naosad Alam, B. K. Agrawal
The model dependence and the symmetry energy dependence of the core-crust transition properties for the neutron stars are studied using three different families of systematically v…
Equation of state of nuclear matter from empirical constraints
N. Alam, B. K. Agrawal, J. N. De +2
From empirically determined values of some of the characteristic constants associated with homogeneous nuclear matter at saturation and sub-saturation densities, within the framewo…