Cosmology with Causal and Non-Causal Dark Viscous Fluid Models - Talole, Rupali S.; Dhankar, Praveen Kumar; Khadekar, G S
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Multiple cosmological observations, including Type Ia supernovae, the Cosmic Microwave Background (CMB), and Baryon Acoustic Oscillations (BAO), confirm the accelerated expansion of the universe. This has prompted the need for theoretical models that go beyond the standard cosmological framework. Among various approaches, the incorporation of bulk viscous effects in the cosmic fluid content has attracted considerable attention. Bulk viscosity serves as an effective mechanism to account for irreversible processes in the cosmological fluid.

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Produktbeschreibung
Multiple cosmological observations, including Type Ia supernovae, the Cosmic Microwave Background (CMB), and Baryon Acoustic Oscillations (BAO), confirm the accelerated expansion of the universe. This has prompted the need for theoretical models that go beyond the standard cosmological framework. Among various approaches, the incorporation of bulk viscous effects in the cosmic fluid content has attracted considerable attention. Bulk viscosity serves as an effective mechanism to account for irreversible processes in the cosmological fluid.
Autorenporträt
Dr. Rupali S. Talole is an accomplished educator with over 16 years of experience in teaching at the junior college level. She currently serves as a faculty member in the Department of Mathematics at Hislop College, Nagpur, a prestigious institution affiliated with Rashtrasant Tukadoji Maharaj Nagpur University.