Investigating stable quark stars in Rastall-Rainbow gravity and their compatibility with gravitational wave observations

• DOI: 10.1016/j.jheap.2024.02.006
• Publication Date: 2024-02-28T16:51:45Z
• Authors: Takol Tangphati; Dhruba Jyoti Gogoi; Anirudh Pradhan; Ayan Banerjee
• Keywords: FOS: Physical sciences; General Relativity and Quantum Cosmology (gr-qc); General Relativity and Quantum Cosmology

We present a stable model for quark stars in Rastall-Rainbow (R-R) gravity. The structure of this configuration is obtained by utilizing an interacting quark matter equation of state. The R-R gravity theory is developed as a combination of two distinct theories, namely, the Rastall theory and the gravity's rainbow formalism. Depending on the model parameters ($\barλ, η, Σ$), the mass-radius relations are numerically computed for modified Tolman-Oppenheimer-Volkoff (TOV) equations with proper boundary conditions. The stability of equilibrium configuration has been checked through the static stability criterion, adiabatic index and the sound velocity. Our calculations predict larger maximum masses for quark stars, and the obtained results are compatible with accepted masses and radii values, including constraints from GW190814 and GW170817 events in all the studied cases.<br/>Accepted for publication in Journal of High Energy Astrophysics, 12 pages, 7 figures<br/>