Curing black hole singularities with local scale invariance

DOI10.1155/2016/6095236zbMath1357.83008arXiv1309.1188OpenAlexW3105549387WikidataQ59122528 ScholiaQ59122528MaRDI QIDQ504685

Predrag Dominis Prester

Publication date: 17 January 2017

Published in: Advances in Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1309.1188

zbMATH Keywords

quantum effectsbaby universe scenarioblack hole singularitieslocal scale invarianceWeyl-invariant dilaton gravity

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Black holes (83C57) Quantum field theory on curved space or space-time backgrounds (81T20) Applications of differential geometry to physics (53Z05) Space-time singularities, cosmic censorship, etc. (83C75) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items (11)

Absence of covariant singularities in pure gravity ⋮ Spherically symmetric black hole solution in mimetic gravity and anti-evaporation ⋮ Ultraviolet-complete quantum field theories with fractional operators ⋮ An issue with the classification of the scalar–tensor theories of gravity ⋮ Singularity crossing, transformation of matter properties and the problem of parametrization in field theories ⋮ Unattainable extended spacetime regions in conformal gravity ⋮ On attractor mechanism of \(\mathrm{AdS}_4\) black holes ⋮ Charged and non-charged black hole solutions in mimetic gravitational theory ⋮ The geometry of black hole singularities ⋮ Black hole evaporation in conformal gravity ⋮ Spacetime completeness of non-singular black holes in conformal gravity

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• Time dependent black holes and scalar hair
• Exact Hairy Black Holes
• Renormalization group flow of Weyl invariant dilaton gravity

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