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20212026
most citedBayesian reconstruction of nuclear matter parameters from the equation of state of neutron star matter

34 citations · 139 across the 12 of their papers we have counts for

collaborators

12 papers

gr-qc2026

Bayesian Inference of Neutron Star Properties in Gravity Using NICER Observations

Sneha Pradhan, N. K. Patra, Kai Zhou +1

In this work, we investigate neutron stars (NSs) in the strong field regime within the framework of symmetric teleparallel gravity, considering three representative models:…

nucl-th2026

Learning the relations between neutron star and nuclear matter properties with symbolic regression

N. K. Patra, Tuhin Malik, Kai Zhou +1

The equation of state (EOS) of dense matter in neutron stars (NSs) remains uncertain, particularly at supra-nuclear densities where complex nuclear interactions and the potential p…

nucl-th2025★ 6 cited

Bayesian Analysis of the Neutron Star Equation of State and Model Comparison: Insights from PSR J0437+4715, PSR J0614+3329, and Other Multi-Physics Data

Sk Md Adil Imam, N. K. Patra

We perform a comprehensive Bayesian analysis to constrain the neutron star (NS) equation of state (EoS) using a wide range of terrestrial and astrophysical data. The terrestrial in…

nucl-th2025★ 9 cited

Inferring the Equation of State from Neutron Star Observables via Machine Learning

N. K. Patra, Tuhin Malik, Helena Pais +3

We have conducted an extensive study using a diverse set of equations of state (EoSs) to uncover strong relationships between neutron star (NS) observables and the underlying EoS p…

nucl-th2024

Calibrating global behaviour of equation of state by combining nuclear and astrophysics inputs in a machine learning approach

Sk Md Adil Imam, Prafulla Saxena, Tuhin Malik +2

We implemented symbolic regression techniques to identify suitable analytical functions that map various properties of neutron stars (NSs), obtained by solving the Tolman-Oppenheim…

nucl-th2024

Bayesian and Principal Component Analyses of Neutron Star Properties

N. K. Patra

A Bayesian method is used in this extensive work to generate a large set of minimally constrained equations of state (EOSs) for matters in neutron stars (NS). These EOSs are analyz…

nucl-th2023★ 13 cited

Establishing connection between neutron star properties and nuclear matter parameters through a comprehensive multivariate analysis

N. K. Patra, Prafulla Saxena, B. K. Agrawal +1

We have attempted to mitigate the challenge of connecting the neutron star (NS) properties with the nuclear matter parameters that describe equations of state (EoSs). The efforts t…

nucl-th2023★ 31 cited

Systematic analysis of the impacts of symmetry energy parameters on neutron star properties

N. K. Patra, Anagh Venneti, Sk Md Adil Imam +2

The impacts of various symmetry energy parameters on the properties of neutron stars (NSs) have been recently investigated, and the outcomes are at variance, as summarized in Table…

nucl-th2023

High-Density behavior of symmetry energy and speed of sound in the dense matter within an effective chiral model

Prashant Thakur, N. K. Patra, T. K. Jha +1

With an effective chiral model, we investigate how the mesonic cross couplings and affect the density content of the symmetry energy and its higher-order slope paramete…

nucl-th2022★ 14 cited

Effect of the -cut potential on the properties of neutron stars with or without a hyperonic core

N. K. Patra, B. K. Sharma, A. Reghunath +2

Motivated by the recent observation of high-mass pulsars (), we employ the -cut potential on the equation of state (EOS) of high-density matter and the pro…

nucl-th2022★ 32 cited

Nearly model-independent constraints on dense matter equation of state in a Bayesian approach

N. K. Patra, Sk Md Adil Imam, B. K. Agrawal +2

We apply Bayesian approach to construct a large number of minimally constrained equations of state (EOSs) and study their correlations with a few selected properties of a neutron s…

nucl-th2021★ 34 cited

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…