Thermodynamic Functions of the Universe in the Presence of Viscosity in the Relativity Theory and Lyra Geometry | ||||
| Sohag Journal of Sciences | ||||
| Article 3, Volume 8, Issue 1, January 2023, Page 7-14 PDF (362.01 K) | ||||
| Document Type: Regular Articles | ||||
| DOI: 10.21608/sjsci.2022.164780.1035 | ||||
 View on SCiNiTO | ||||
| Authors | ||||
E. A. Hegazy   ; M. Abdel-Megied; Amira A. Gedamy
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| Mathematics Department, Faculty of Science, Minia University, 61519 El-Minia, EGYPT | ||||
| Abstract | ||||
| This paper investigates the thermodynamic functions of the universe in the presence of viscous fluid in general relativity and Lyra geometry. The space-time is modeled by Bianchi type VI_0 cosmological model. The field equations' solution is obtained considering that the scalar expansion θ of the cosmological model is proportional to the eigenvalue σ_1^1 of the shear tensor σ_i^j. The thermodynamic functions are studied for the universe and their values are compared in general relativity and Lyra geometry. For all obtained models, the entropy is consistent with the second law of thermodynamics. The physical and geometrical properties of the obtained models are discussed. Also, we show that the Lyra term β plays the role of the variable cosmological term in the relativity theory and can not be identified as a viscosity term. Without the viscosity term, we obtain the entropy as a constant S= constant. That is the universe is in an adiabatic state. The Bianchi type VI_0 cosmological model presented in this paper explains a stage of evolution with the positive deceleration parameter. | ||||
| Keywords | ||||
| Lyra geometry; Bianchi type $VI_0$ cosmological model; Viscosity; Energy momentum tensor; Thermodynamic functions | ||||
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