Anisotropic Cosmological Model with a Generalized Chaplygin Gas
Anisotropic Cosmological Model with a Generalized Chaplygin Gas
Anisotropic Cosmological Model with a Generalized Chaplygin Gas
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•(d) Acceleration due to non gravitational force like pressure gradientis a vector defined by!Ya= Ya;bYbwhich is orthogonal toY a*The trace of the tidal tensor (Raychaudhury scalar)(if positive we call it the strong energy condition)ˆ $ #R Y Y = 4"G(! +$#3P).