An approximate solution of gravitational equations of expanding universe

Physics

Scientific paper

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Scientific paper

Einstein's gravitational equations of expanding universe is solved by neglecting cosmological terms. On assumption P=1/3ϱ the value of ƒ;(t) and ϱ (density) are calculated {ƒ;(t) = -4k2t2+ct+D and ϱ = γ/(-4k2t2+ct+D)2} It shows the possibility of sudden collaps of the expanding universe into zero volume with infinite density at that stage.

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