Journals / Turkish Journal of Physics / 2007 / Cilt: 31 - Sayı: 2

Bianchi Type VI1 Viscous Fluid Cosmological Model in Wesson´s Theory of Gravitation

Pages
59–66
Publication Date
2007-02-01
DOI
—
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AI Summary & Key Takeaways

AI Insight
⚡ TL;DR(Too Long; Didn't Read)

We have discussed some physical and kinematical properties of the models.

📌 3 Key Takeaways

🎯
Objective & Hypothesis:Field equations of a scale invariant theory of gravitation proposed by Wesson [1, 2] are obtained in the presence of viscous fluid with the aid of Bianchi type VIh space-time with the time dependent gauge function (Dirac gauge).
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Key Findings & Data:It is found that Bianchi type VIh (h = 1) space-time with viscous fluid is feasible in this theory, whereas Bianchi type VIh (h = -1, 0) space-times are not feasible in this theory, even in the presence of viscosity.
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Conclusion & Impact:We have discussed some physical and kinematical properties of the models.
🔬Design:Modeling & Simulation
📍Scope:Comprehensive Sample
⚙️Variables:Gauge function · viscous fluid · scale invariant theory.

Abstract

Field equations of a scale invariant theory of gravitation proposed by Wesson [1, 2] are obtained in the presence of viscous fluid with the aid of Bianchi type VIh space-time with the time dependent gauge function (Dirac gauge). It is found that Bianchi type VIh (h = 1) space-time with viscous fluid is feasible in this theory, whereas Bianchi type VIh (h = -1, 0) space-times are not feasible in this theory, even in the presence of viscosity. For the feasible case, by assuming a relation connecting viscosity and metric coefficient, we have obtained a nonsingular-radiating model. We have discussed some physical and kinematical properties of the models.

Özet

Field equations of a scale invariant theory of gravitation proposed by Wesson [1, 2] are obtained in the presence of viscous fluid with the aid of Bianchi type VIh space-time with the time dependent gauge function (Dirac gauge). It is found that Bianchi type VIh (h = 1) space-time with viscous fluid is feasible in this theory, whereas Bianchi type VIh (h = -1, 0) space-times are not feasible in this theory, even in the presence of viscosity. For the feasible case, by assuming a relation connecting viscosity and metric coefficient, we have obtained a nonsingular-radiating model. We have discussed some physical and kinematical properties of the models.

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Cite This Article

KHADEKAR, G. S., AVACHAR, G. R. (2007). Bianchi Type VI1 Viscous Fluid Cosmological Model in Wesson´s Theory of Gravitation. Turkish Journal of Physics, Cilt: 31 - Sayı: 2, 59–66. https://ajindex.com/articles/724080

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