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20212026
most citedNearly model-independent constraints on dense matter equation of state in a Bayesian approach

32 citations · 105 across the 11 of their papers we have counts for

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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…