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Alternative for Black Hole Paradoxes

Published 20 May 2022 in hep-th and gr-qc | (2205.10437v2)

Abstract: A throughout investigation is made of the exact black hole solution in five-dimensional warped conformal dilaton gravity, found in an earlier investigation. The singularities of the dynamical black hole spacetime are determined by the zeros of a meromorphic quintic polynomial, which has no essential singularities. The solutions of the polynomial are analyzed in the complex plane in relation to the icosahedron group and by the Hopf-fibrations of the Klein surface. The model fits the antipodal boundary condition, i.e., antipodal points in the projected space are identified using the embedding of a Klein surface in $\mathds{C}2$, using the $\mathds{Z}2$ symmetry on the two sides of the brane. If one writes ${(5)}g{\mu\nu}=\omega{4/3}{{(5)}}{\tilde g_{\mu\nu}}, {{(5)}}{\tilde g_{\mu\nu}}={{(4)}}{\tilde g_{\mu\nu}}+n_\mu n_\nu$, $ {(4)}\tilde g_{\mu\nu}=\bar\omega2 {{(4)}}\bar g_{\mu\nu}$, with $n_\mu$ the normal to the brane and $\omega$ the dilaton field, then ${{(4)}}\bar g_{\mu\nu}$ is conformally flat. It is the contribution from the bulk which determines the real pole on the effective four-dimensional spacetime. There is no objection applying 't Hooft's back reaction method in constructing the unitary S-matrix for the Hawking radiation. Again, there is no "inside" of the black hole.

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