Constraining a relativistic mean field model using neutron star mass–radius measurements II: hyperonic models

ABSTRACT We investigate whether measurements of the neutron star mass and radius or the tidal deformability can provide information about the presence of hyperons inside a neutron star. This is achieved by considering two inference models, with and without hyperons, based on a field theoretical approach. While current observations do not distinguish between the two scenarios, we have shown that data simulating expected observations from future large-area X-ray timing telescopes could provide some information through Bayes’ factors. Inference using simulated data generated from an equation of state containing hyperons decisively favours the hyperonic model over the nucleonic model. However, a 2 per cent uncertainty in the mass and radius determination may not be sufficient to constrain the parameters of the model when only six neutron star mass–radius measurements are considered.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2024-12-20
DOI
https://doi.org/10.1093/mnras/stae2792
Citations
19
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
6.30

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article

Constraining a relativistic mean field model using neutron star mass–radius measurements II: hyperonic models

Anna L. Watts, Constança Providência, Laura Tolós, Chun Huang
19 citations
Monthly Notices of the Royal Astronomical Society
Pulsars and Gravitational Waves Research
6.30
article

Constraining a relativistic mean field model using neutron star mass–radius measurements II: hyperonic models

Anna L. Watts, Constança Providência, Laura Tolós, Chun Huang
article en
19 citations

Abstract

ABSTRACT We investigate whether measurements of the neutron star mass and radius or the tidal deformability can provide information about the presence of hyperons inside a neutron star. This is achieved by considering two inference models, with and without hyperons, based on a field theoretical approach. While current observations do not distinguish between the two scenarios, we have shown that data simulating expected observations from future large-area X-ray timing telescopes could provide some information through Bayes’ factors. Inference using simulated data generated from an equation of state containing hyperons decisively favours the hyperonic model over the nucleonic model. However, a 2 per cent uncertainty in the mass and radius determination may not be sufficient to constrain the parameters of the model when only six neutron star mass–radius measurements are considered.

Monthly Notices of the Royal Astronomical SocietyVol. 536(4)
Institute of Space Sciences (ES), Washington University in St. Louis (US), Frankfurt Institute for Advanced Studies (DE), Institut d'Estudis Espacials de Catalunya (ES), Astronomical Institute of the Slovak Academy of Sciences (SK), University of Coimbra (PT), University of Amsterdam (NL)
National Aeronautics and Space Administration, Washington University in St. Louis, Strong, European Commission, Generalitat de Catalunya, Federación Española de Enfermedades Raras, Generalitat Valenciana, Nuclear Safety and Security Commission, Ministerio de Ciencia e Innovación, Horizon 2020 Framework Programme, Fundação para a Ciência e a Tecnologia, Agencia Estatal de Investigación, H2020 European Research Council
Openalex Percentile: Top 3%
Pulsars and Gravitational Waves Research
6.30
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