Bayesian Exploration of Phenomenological EoS of Neutron/Hybrid Stars with Recent Observations
Abstract
The description of the stellar interior of compact stars remains as a big challenge for the nuclear astrophysics community. The consolidated knowledge is restricted to density regions around the saturation of hadronic matter ρ0=2.8 × 1014 g cm-3, regimes where our nuclear models are successfully applied. As one moves towards higher densities and extreme conditions up to the quark/gluons deconfinement, little can be said about the microphysics of the equation of state (EoS). Here, we employ a Markov Chain Monte Carlo (MCMC) strategy to access the variability at high density regions of polytropic piecewise models for neutron star (NS) EoS or possible hybrid stars, i.e., a NS with a small quark-matter core. With a fixed description of the hadronic matter for low density, below the nuclear saturation density, we explore a variety of models for the high density regimes leading to stellar masses near to 2.5 M⊙, in accordance with the observations of massive pulsars. The models are constrained, including the observation of the merger of neutrons stars from VIRGO-LIGO and with the pulsar observed by NICER. In addition, we also discuss the possibility of the use of a Bayesian power regression model with heteroscedastic error. The set of EoSmore »
- Authors:
-
- Brookhaven National Lab. (BNL), Upton, NY (United States). National Nuclear Data Center (NNDC)
- Texas A & M Univ., Commerce, TX (United States); University of the Andes (Colombia)
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Texas A & M Univ., Commerce, TX (United States)
- Publication Date:
- Research Org.:
- Brookhaven National Laboratory (BNL), Upton, NY (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Nuclear Physics (NP)
- OSTI Identifier:
- 1974190
- Report Number(s):
- BNL-224285-2023-JAAM
Journal ID: ISSN 2571-712X; TRN: US2313944
- Grant/Contract Number:
- SC0012704; FG02-08ER41533; AC02-98CH10886
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Particles
- Additional Journal Information:
- Journal Volume: 6; Journal Issue: 1; Journal ID: ISSN 2571-712X
- Publisher:
- MDPI
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 73 NUCLEAR PHYSICS AND RADIATION PHYSICS; Bayesian inference; MCMC; equation of state; neutron star; astrophysics
Citation Formats
Chimanski, Emanuel V., Lobato, Ronaldo V., Goncalves, Andre R., and Bertulani, Carlos A. Bayesian Exploration of Phenomenological EoS of Neutron/Hybrid Stars with Recent Observations. United States: N. p., 2023.
Web. doi:10.3390/particles6010011.
Chimanski, Emanuel V., Lobato, Ronaldo V., Goncalves, Andre R., & Bertulani, Carlos A. Bayesian Exploration of Phenomenological EoS of Neutron/Hybrid Stars with Recent Observations. United States. https://doi.org/10.3390/particles6010011
Chimanski, Emanuel V., Lobato, Ronaldo V., Goncalves, Andre R., and Bertulani, Carlos A. Thu .
"Bayesian Exploration of Phenomenological EoS of Neutron/Hybrid Stars with Recent Observations". United States. https://doi.org/10.3390/particles6010011. https://www.osti.gov/servlets/purl/1974190.
@article{osti_1974190,
title = {Bayesian Exploration of Phenomenological EoS of Neutron/Hybrid Stars with Recent Observations},
author = {Chimanski, Emanuel V. and Lobato, Ronaldo V. and Goncalves, Andre R. and Bertulani, Carlos A.},
abstractNote = {The description of the stellar interior of compact stars remains as a big challenge for the nuclear astrophysics community. The consolidated knowledge is restricted to density regions around the saturation of hadronic matter ρ0=2.8 × 1014 g cm-3, regimes where our nuclear models are successfully applied. As one moves towards higher densities and extreme conditions up to the quark/gluons deconfinement, little can be said about the microphysics of the equation of state (EoS). Here, we employ a Markov Chain Monte Carlo (MCMC) strategy to access the variability at high density regions of polytropic piecewise models for neutron star (NS) EoS or possible hybrid stars, i.e., a NS with a small quark-matter core. With a fixed description of the hadronic matter for low density, below the nuclear saturation density, we explore a variety of models for the high density regimes leading to stellar masses near to 2.5 M⊙, in accordance with the observations of massive pulsars. The models are constrained, including the observation of the merger of neutrons stars from VIRGO-LIGO and with the pulsar observed by NICER. In addition, we also discuss the possibility of the use of a Bayesian power regression model with heteroscedastic error. The set of EoS from the Laser Interferometer Gravitational-Wave Observatory (LIGO) was used as input and treated as the data set for the testing case.},
doi = {10.3390/particles6010011},
journal = {Particles},
number = 1,
volume = 6,
place = {United States},
year = {Thu Feb 02 00:00:00 EST 2023},
month = {Thu Feb 02 00:00:00 EST 2023}
}
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