THE AFFINITY BETWEEN THE EVENT HORIZON DERIVED FROM HOWUSU METRIC TENSOR AND THAT OF THE SCHWARZSCHILD METRIC TENSOR
Abstract
A black hole is an object so dense that it sufficiently bends the space-time around it so that nothing can escape. The maximum distance from the center of the black hole for which nothing can escape is called the event horizon. This was first calculated by
Schwarzschild metric tensor. In this paper, the Howusu metric tensor for all gravitational fields in nature has been used to calculate the event horizon of a black hole and it is found that ???? = ???? ,which is the same as that of the Schwarzschild metric tensor.
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Hoyle, F.(1948).A new model for the expanding universe. Monthly Notices of the Royal Astronomical Society.108: 372-382.
Zhang T.X. (2009) A new cosmological model: Black Hole Universe. Progress in Physics. 3:4-5
Howusu S. X. K. (2009). The metric tensors for gravitational fields and the mathematical principles of Riemannian theoretical physics Jos: Jos University press.Pp26-28
Howusu, S.X.K. (2012) The Super Golden Metric tensors in orthogonal curvilinear coordinates. Jos: Jos University press. Pp 1-2
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