2002
DOI: 10.1023/a:1015858621340
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Cited by 9 publications
(5 citation statements)
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“…On integration, (2.20) yields two basic solutions for φ as The energy density ρ associated with the massless scalar field ν (Mohanty [17,18]; Panigrahi and Sahu [19]) is given by (2.13)] that rest energy density (for strings) ε = 0. Hence particle density (for strings) ε p = 0.…”
Section: Field Equations and Modelmentioning
confidence: 99%
“…On integration, (2.20) yields two basic solutions for φ as The energy density ρ associated with the massless scalar field ν (Mohanty [17,18]; Panigrahi and Sahu [19]) is given by (2.13)] that rest energy density (for strings) ε = 0. Hence particle density (for strings) ε p = 0.…”
Section: Field Equations and Modelmentioning
confidence: 99%
“…Singh and Deo [3], Reddy [4][5][6], Maharaj and Beesham [7], Venkateswarlu and Reddy [8][9][10], Shanti and Rao [11], Mohanty et al [12,13] are some of the authors who have investigated various aspects of Barber's self creation theories. Mohanty et al [14] have obtained a micro and macro cosmological models in the presence of massless scalar field interacted with perfect fluid. Panigrahi and Sahu [15][16][17] have also obtained plane symmetric inhomogeneous cosmological micro and macro models and plane symmetric mesonic stiff fluid models in Barber's second theory of gravitation.…”
Section: Introductionmentioning
confidence: 99%
“…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.…”
Section: Introductionmentioning
confidence: 99%