Conformal Dilaton-Higgs Gravity on Warped Spacetimes: Black Hole Paradoxes revisited
Reinoud Jan Slagter

TL;DR
This paper explores a conformal dilaton-Higgs gravity model on warped spacetimes, providing new insights into black hole solutions, antipodal boundary conditions, and their implications for the information paradox, with potential advantages in describing Hawking radiation.
Contribution
It introduces a novel Kerr-like black hole solution in a conformal dilaton-Higgs gravity framework on warped spacetimes, emphasizing antipodal boundary conditions and their role in black hole information paradoxes.
Findings
Effective 4D brane spacetime derived from 5D manifold
Antipodal boundary condition maintains symmetry without quantum cloning
Relation established between Klein surface embedding and information paradox
Abstract
We investigate on a Randall-Sundrum warped spacetime, a Kerr-like black hole in the conformal dilaton-Higgs gravity model. We applied the antipodal boundary condition on the Klein surface using the -symmetry in the "large" (bulk) extra dimension. It turns out that the pseudo-Riemannian 5D manifold can be written as an effective 4D Riemannian brane spacetime, , where is conformally flat. The solution in valid on both manifolds. So the solution can equally well described by an instanton solution. An advantage is that antipodicity can be maintained without a "cut-and-past" method or to rely on quantum cloning, when treating the scattering description of the evaporation process of the Hawking radiation. We need only the windingnumber as quantum number. Moreover, the equations are invariant under time…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories · Relativity and Gravitational Theory
