Axially Symmetric Cosmological Micro Model in Barber’s Modified Theory of Einstein General Relativity

Abstract

Axially symmetric Bianchi type-I cosmological micro model is obtained in Barber's (Gen. Relativ. Gravit. 14:117, 1982) modified theory of general relativity. Some properties of the model are discussed.

Axially Symmetric Bianchi Type-I Model with Massless Scalar Field and Cosmic Strings in Barber’s Self-Creation Cosmology

“…(2.29) Above model is similar to the model obtained by Adhav et al [27]. The metric potentials A and B tend to zero as T → 0.…”

“…The study of string cosmological models was initiated by Vilenkin [22], Letelier [23], Krori et al [24]. Bhattacharjee and Baruah [25], Reddy [26], Adhav et al [27] studied the problem of comic strings in Bianchi type cosmologies with a self-interacting scalar field.…”

Wet Dark Fluid Cosmological Model in Barber Self-Creation Theory of Gravitation

“…Many authors [3][4][5][6][7][8][9][10][11][12] have investigated various aspects of Barber second self-creation theory by using various cosmological models.…”