| viXra.org > Relativity and Cosmology > viXra:2606.0027 |
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| viXra.org > Relativity and Cosmology > viXra:2606.0027 |
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Relativity and Cosmology |
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Authors: Tanishq Chandu Khandare
I derive a non-vanishing, solution to the Einstein-Maxwell field equations representing a dynamical, radiating, rotating, and charged manifold. Utilizing the Newman-Penrose (NP) formalist, I project the metric onto a nulltetrad {l, n, m, m¯ } to evaluate the Weyl and Ricci scalars. We demonstrate that the resulting stress-energy tensor Tµν = T (null) µν + T(em) µν satisfies the Weak Energy Condition (WEC) and the local conservation law ∇µTµν = 0. By formalizing the EPR criterion for physical completeness, we argue that the stationary KerrNewman limit is a sub-manifold of the broader radiative reality. I further prove that the r = 0 singularity is a transient topological feature that resolves into a Minkowski vacuum in the limit of total evaporation.
Comments: 2 Pages.
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[v1] 2026-06-08 19:46:29
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