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G. P. Singh and J. Singh, “String Cosmological Models with Magnetic Field,” General Relativity Gravitation, Vol. 31, No. 3, 1999, pp. 371-378. doi:10.1023/A:1026644828215

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.