String Cosmology in Bulk Viscous Bianchi Type – III Space-Time

Exploring the Physical and Geometrical Features of a Bulk Viscous String Cosmological Model

Authors

  • Dr. Sunil Suman
  • Brajesh Kumar

Keywords:

string cosmology, bulk viscous, Bianchi type-III, solution, scalar of expansion

Abstract

The present paper provides solution of Bianchi type- III bulk viscous string cosmological model of assuming that (i) ξ2 = μ2θ and (ii) σ ∞ θ which leads to β = γζ (where μ and ζ are constants, ζ is bulk viscosity and θ is scalar of expansion). Various physical and geometrical features of the model are also found and discussed.

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Published

2021-04-01

How to Cite

[1]
“String Cosmology in Bulk Viscous Bianchi Type – III Space-Time: Exploring the Physical and Geometrical Features of a Bulk Viscous String Cosmological Model”, JASRAE, vol. 18, no. 3, pp. 421–424, Apr. 2021, Accessed: May 10, 2025. [Online]. Available: https://ignited.in/index.php/jasrae/article/view/13143

Issue

Vol. 18 No. 3 (2021): Journal of Advances and Scholarly Researches in Allied Education (JASRAE)

Section

Articles

How to Cite

[1]
“String Cosmology in Bulk Viscous Bianchi Type – III Space-Time: Exploring the Physical and Geometrical Features of a Bulk Viscous String Cosmological Model”, JASRAE, vol. 18, no. 3, pp. 421–424, Apr. 2021, Accessed: May 10, 2025. [Online]. Available: https://ignited.in/index.php/jasrae/article/view/13143