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R. Bali and S. Dave, “Bianchi Type-III String Cosmological Models with Bulk Viscous Fluid in General Relativity,” Astrophysics and Space Science, Vol. 282, No. 1, 2002, pp. 461-467.

has been cited by the following article:

• TITLE: Cosmic String in Bianchi Type-III Space-Time with Bulk Viscosity and Magnetic Field

  AUTHORS: Sharad Panditrao Kandalkar, Amrapali Pandurang Wasnik, Sunita Padmakar Gawande, Mohini Nilkanth Gaikwad

  KEYWORDS: Bulk Viscosity; Magnetic Field; String Cosmological

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.2 No.4, December 31, 2012

  ABSTRACT: We investigate some locally rotationally symmetric (LRS) Bianchi type-III string cosmological model in the presence of bulk viscosity and magnetic field, where an equation of state and relation between metric potential are considered. The solution describes a shearing and non-rotating model with big-bang start. In the absence of magnetic field it reduces to a string model with bulk viscosity, where the relation between the coefficient of bulk viscosity and the energy density is for a = 0.