402 citations · 897 across the 24 of their papers we have counts for
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Density dependence of symmetry energy and neutron skin thickness revisited using relativistic mean field models with nonlinear couplings
Chiranjib Mondal
The correlation between neutron skin-thickness of a neutron-rich nucleus and slope parameter of symmetry energy is assessed as a function of density using relativistic mean field m…
Can we decipher the composition of the core of a neutron star?
Chiranjib Mondal, Francesca Gulminelli
General relativity guarantees a unique one-to-one correspondence between static observables of neutron stars (NSs) accessible by multi-messenger astronomy, such as mass-radius or t…
Bayesian reconstruction of nuclear matter parameters from the equation of state of neutron star matter
Sk Md Adil Imam, N. K. Patra, C. Mondal +2
The nuclear matter parameters (NMPs), those underlie in the construction of the equation of state (EoS) of neutron star matter, are not directly accessible. The Bayesian approach i…
The nuclear matter density functional under the nucleonic hypothesis
Hoa Dinh Thi, Chiranjib Mondal, Francesca Gulminelli
A Bayesian analysis of the possible behaviors of the dense matter equation of state informed through recent LIGO-Virgo as well as NICER measurements reveals that all the present ob…
Unified Equation of State for Neutron Stars Based on the Gogny Interaction
Xavier Viñas, Claudia Gonzalez-Boquera, Mario Centelles +2
The most popular Gogny parametrizations, namely D1S, D1N and D1M, describe accurately the ground-state properties of spherical and deformed finite nuclei all across the mass table…
Analysis of critical parameters for nonrelativistic models in symmetric nuclear matter
Mariana Dutra, Odilon Lourenço, Xavier Viñas +1
In this work we have analyzed several features of symmetric nuclear matter (SNM) at finite temperature described by different zero- and finite-range nonrelativistic families of mod…