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
1. Verfasser:	Korunur, Sibel
Format:	Artikel
Sprache:	eng
Schlagworte:	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
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Zusammenfassung:	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.
ISSN:	0001-7701 1572-9532
DOI:	10.1007/s10714-023-03188-3