Charged quark stars in gravity
arXiv:2207.12947 · doi:10.1088/1674-1137/ac84cb
Abstract
Recent advances in nuclear theory combined with new astrophysical observations have led to the need for specific theoretical models that actually apply to phenomena on dense-matter physics. At the same time, quantum chromodynamics (QCD) predicts the existence of non-nucleonic degrees of freedom at high densities in neutron-star matter, such as quark matter. Within a confining quark matter model, which consists of homogeneous, neutral 3-flavor interacting quark matter with corrections, we study the structure of compact stars made of a charged perfect fluid in the context of gravity. The system of differential equations that describe the structure of charged compact stars have been derived and solved numerically for a gravity model with . For simplicity, we assume that the charge density is proportional to the energy density, namely, . It is demonstrated that matter-geometry coupling constant and the charge parameter affect the total gravitational mass and the radius of the star.
10 pages, 6 figures. To appear in Chinese Physics C
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- Dynamical reconstruction of the CDM model in scalar-tensor gravity
- Moment of inertia and compactness of quark stars within the context of gravity
- Relativistic structure of charged quark stars in energy-momentum squared gravity
- Neutron Stars in Modified Teleparallel Gravity
- The Reconstruction of Constant Jerk Parameter with Gravity in Bianchi-I spacetime
- Neutron Stars In Theory: Slow Rotation Approximation
- Stellar structure in gravity: some exact solutions
- Constraint on the equation of state of strange quark star: Perturbative QCD along with a density-dependent bag constant
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