Sharma–Mittal holographic dark energy and scalar field in Bianchi type-I cosmology

In this work, we studied Sharma–Mittal holographic dark energy model by considering Bianchi type-I cosmology. For this purpose we analyzed equation of state parameter using IR cutoff scale. Also it is reconstructed correspondence between Sharma–Mittal holographic dark energy and tachyon and quintess...

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Veröffentlicht in:General relativity and gravitation 2024, Vol.56 (1), Article 2
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description In this work, we studied Sharma–Mittal holographic dark energy model by considering Bianchi type-I cosmology. For this purpose we analyzed equation of state parameter using IR cutoff scale. Also it is reconstructed correspondence between Sharma–Mittal holographic dark energy and tachyon and quintessence scalar fields. Finally, we created plots for the time-evolution of the equation of state, kinetic energy, and scalar potential.
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subjects Astronomy
Astrophysics and Cosmology
Classical and Quantum Gravitation
Cosmology
Dark energy
Differential Geometry
Equations of state
Holography
Kinetic energy
Mathematical and Computational Physics
Physics
Physics and Astronomy
Quantum Physics
Quintessence (cosmology)
Relativity Theory
Scalars
Theoretical
title Sharma–Mittal holographic dark energy and scalar field in Bianchi type-I cosmology
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