Behavior of Magnetized Strange Quark Matter in 5D Cosmological Model

Aktaş, Can; Aktaş, Can B.

doi:10.1007/s40995-022-01363-w

Cited by 3 publications

(1 citation statement)

References 41 publications

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“…Aygün et al [12] have investigated scalar field solutions both Lyra geometry and Riemannian geometry for Marder space-time. Kalkan and Aktaş [13] have studied MSQM for 5D Kaluza-Klein metric in f (R, T ) theory. The behavior of MSQM was investigated by Kalkan et al [14] within the framework of f (R, T ) theory in inhomogeneous anisotropic space-time.…”

Section: Introductionmentioning

confidence: 99%

Magnetized Strange Quark Models in Lyra Theory

Aktaş

2023

Journal of New Theory

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In this study, the behavior of magnetized strange quark matter (MSQM) distribution in Lyra theory was investigated for homogeneous anisotropic Bianchi III, locally rotationally symmetric (LRS) Bianchi I, and Kantowski-Sachs universe models. We have used the equations of state, anisotropy, and linearly varying deceleration parameters to obtain the exact solutions of field equations in Lyra theory. When switching from the anisotropic universe model to the isotropic universe model, the magnetic field was not observed in the LRS Bianchi I universe. Besides, the graphs of the dynamic quantities obtained for each universe model were analyzed in detail. Finally, we inquire whether further research should be conducted.

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Section: Introductionmentioning

confidence: 99%

Magnetized Strange Quark Models in Lyra Theory

Aktaş

2023

Journal of New Theory

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Magnetic string matter collapse in rainbow gravity

Tasleem,

Sheikh

2024

Can. J. Phys.

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This work investigates the dynamics of a collapsing magnetic string dust and string fluid in the Plank Era via spherically symmetric rainbow geometry. The field equations are modified and solved to obtain the dynamical quantities including mass density, pressure, string tension, and magnetic field strength. These quantities are presented graphically. The energy conditions are computed showing that all the dynamical quantities are associated with physical matter. The distance and moment of apparent horizon formation are computed. The magnetic field is found to affect the distance and moment of the apparent horizon's formation. It accelerates the collapsing process. Further, the dynamical variables are maximum in the collapsing configuration's center leading to compact object (black hole) formation. The probing particle's energy affects all the dynamical variables of the fluid in a direct proportion. This resolves the information paradox as a particle with greater energy grasps the information from a particle with lesser energy and takes it out in the real world.

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Compact object formation from collapsing magnetized strange quark matter in rainbow gravity

Tasleem,

Sheikh,

Ali

2023

Int. J. Geom. Methods Mod. Phys.

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This study focuses on the dynamics of magnetized strange quark matter collapsing near a star in rainbow gravity. The study computes various dynamical variables, including mass density, pressure, and magnetic field strength, to ensure the physical existence of the fluid, and graphically verifies the energy conditions. These variables combine to form a black hole, and the study estimates the time and distance of apparent horizon formation, which are both reduced by the magnetic field. Additionally, the study observes that the energy of probing particles impacts mass density, pressure, magnetic field intensity, distance, and time of horizon creation, which helps to resolve the information paradox. It is also noticed that the magnetic field accelerates the collapse.

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Behavior of Magnetized Strange Quark Matter in 5D Cosmological Model

Cited by 3 publications

References 41 publications

Magnetized Strange Quark Models in Lyra Theory

Magnetized Strange Quark Models in Lyra Theory

Magnetic string matter collapse in rainbow gravity

Compact object formation from collapsing magnetized strange quark matter in rainbow gravity

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