Relativistic structure of charged quark stars in energy-momentum squared gravity
Juan M. Z. Pretel, Takol Tangphati, Ayan Banerjee

TL;DR
This paper explores how energy-momentum squared gravity (EMSG) affects the structure and maximum mass of charged quark stars, revealing that different matter Lagrangians and charge distributions significantly influence stellar properties.
Contribution
It derives modified TOV equations in EMSG for charged stars, compares effects of different matter Lagrangians, and numerically analyzes mass-radius relations with electric charge.
Findings
Maximum mass varies with gravity parameter and matter Lagrangian choice.
Electric charge influences the mass-radius relationship significantly.
Behavior of maximum mass with gravity parameter is complex and depends on matter Lagrangian.
Abstract
Within the context of energy-momentum squared gravity (EMSG), where non-linear matter contributions appear in the gravitational action, we derive the modified TOV equations describing the hydrostatic equilibrium of charged compact stars. We adopt two different choices for the matter Lagrangian density ( versus ) and investigate the impact of each one on stellar structure. Furthermore, considering a charge profile where the electric charge density is proportional to the standard energy density , we solve numerically the stellar structure equations in order to obtain the mass-radius diagrams for the MIT bag model equation of state (EoS). For and given a specific value of (including the uncharged case when ), the maximum-mass values increase (decrease) substantially as the gravity model…
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