Thermal effects on the baryon–quark phase transition in hot hybrid neutron stars: a statistical mean-field baryonic model with the standard NJL model for deconfined quarks

Ghaemmaghami, S. A.; Ghazanfari Mojarrad, M.

doi:10.1140/epjp/s13360-023-04611-z

Eur. Phys. J. Plus

2023

DOI: 10.1140/epjp/s13360-023-04611-z

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Thermal effects on the baryon–quark phase transition in hot hybrid neutron stars: a statistical mean-field baryonic model with the standard NJL model for deconfined quarks

S. A. Ghaemmaghami,

M. Ghazanfari Mojarrad

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2024

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Properties of interacting quark star in light of Rastall gravity

Banerjee,

Pradhan,

Sakallı

et al. 2024

Class. Quantum Grav.

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This study explores the properties of quark stars (QS) formulated with an interacting quark matter equation of state (EoS) within the framework of Rastall gravity, a modified theory of gravity. We derive the mass-radius relationships and calculate the maximum gravitational masses and their corresponding radii, comparing these results under both Rastall gravity and general relativity. Our analysis incorporates recent observational data, including the GW190425 event, to constrain the model parameters ($\bar{\lambda}, \eta, B_{\rm eff}$). We also assess the stability of these quark stars by evaluating their static stability, adiabatic index, and sound velocity profiles, \textcolor{blue}{thus confirming their viability within the modified gravitational framework}.

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Properties of interacting quark star in light of Rastall gravity

Banerjee,

Pradhan,

Sakallı

et al. 2024

Class. Quantum Grav.

View full text Add to dashboard Cite

show abstract

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Thermal effects on the baryon–quark phase transition in hot hybrid neutron stars: a statistical mean-field baryonic model with the standard NJL model for deconfined quarks

Cited by 1 publication

References 95 publications

Properties of interacting quark star in light of Rastall gravity

Properties of interacting quark star in light of Rastall gravity

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