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of 57
pro vyhledávání: '"Patra, N. K."'
We implemented symbolic regression techniques to identify suitable analytical functions that map various properties of neutron stars (NSs), obtained by solving the Tolman-Oppenheimer-Volkoff (TOV) equations, to a few key parameters of the equation of
Externí odkaz:
http://arxiv.org/abs/2407.08553
Autor:
Patra, N. K.
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 analyzed for their correlations with key NS properties, such as the tidal de
Externí odkaz:
http://arxiv.org/abs/2404.17248
Publikováno v:
Phys. Rev. D (2023)
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 to correlate various neutron star properties with individual nuclear ma
Externí odkaz:
http://arxiv.org/abs/2308.13896
Publikováno v:
Phys. Rev. C (2023)
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 III of Phys. Rev. D 106, 063005 (2022). We have systematically analyz
Externí odkaz:
http://arxiv.org/abs/2302.03906
With an effective chiral model, we investigate how the mesonic cross couplings $\sigma-\rho$ and $\omega-\rho$ affect the density content of the symmetry energy and its higher-order slope parameters. Earlier mentioned cross-couplings are crucial to c
Externí odkaz:
http://arxiv.org/abs/2301.12690
Publikováno v:
Phys. Rev. C (2022)
Motivated by the recent observation of high-mass pulsars ($M \simeq 2 M_{\odot}$), we employ the $\sigma$-cut potential on the equation of state (EOS) of high-density matter and the properties of neutron stars within the relativistic mean-field (RMF)
Externí odkaz:
http://arxiv.org/abs/2211.10616
Publikováno v:
Phys. Rev. D 106, 043024 (2022)
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 star (NS). Our set of minimal constraints includes a few basic properti
Externí odkaz:
http://arxiv.org/abs/2203.08521
Publikováno v:
Phys. Rev. C 105, 015806 (2022)
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 is applied to reconstruct the posterior distributions of NMPs from the
Externí odkaz:
http://arxiv.org/abs/2110.15776
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