Regular black holes: A short topic review
C Lan, H Yang, Y Guo, YG Miao - International Journal of Theoretical …, 2023 - Springer
The essential singularity in Einstein's gravity can be avoidable if the preconditions of
Penrose's theorem can be bypassed, ie, if the strong energy condition is broken in the …
Penrose's theorem can be bypassed, ie, if the strong energy condition is broken in the …
[PDF][PDF] Fundamental physics opportunities with the next-generation event horizon telescope
D Ayzenberg, L Blackburn, R Brito… - arXiv preprint arXiv …, 2023 - researchgate.net
Abstract The Event Horizon Telescope (EHT) Collaboration recently published the first
images of the supermassive black holes in the cores of the Messier 87 and Milky Way …
images of the supermassive black holes in the cores of the Messier 87 and Milky Way …
Quantum oppenheimer-snyder and swiss cheese models
By considering the quantum Oppenheimer-Snyder model in loop quantum cosmology, a
new quantum black hole model whose metric tensor is a suitably deformed Schwarzschild …
new quantum black hole model whose metric tensor is a suitably deformed Schwarzschild …
Mass inflation without Cauchy horizons
Mass inflation is a well established instability, conventionally associated to Cauchy horizons
(which are also inner trapping horizons) of stationary geometries, leading to a divergent …
(which are also inner trapping horizons) of stationary geometries, leading to a divergent …
Regular black holes without mass inflation instability
A bstract Generic models of regular black holes have separate outer and inner horizons,
both with nonzero surface gravity. It has been shown that a nonzero inner horizon surface …
both with nonzero surface gravity. It has been shown that a nonzero inner horizon surface …
Quasinormal modes-shadow correspondence for rotating regular black holes
D Pedrotti, S Vagnozzi - Physical Review D, 2024 - APS
Eikonal quasinormal modes (QNMs) of black holes (BHs) and parameters of null geodesics,
ultimately tied to the appearance of BHs to external observers, are known to be related, and …
ultimately tied to the appearance of BHs to external observers, are known to be related, and …
Geometry of the black-to-white hole transition within a single asymptotic region
We write explicitly the complete Lorentzian metric of a singularity-free spacetime where a
black hole transitions into a white hole located in its same asymptotic region. In particular …
black hole transitions into a white hole located in its same asymptotic region. In particular …
Scalar perturbations around rotating regular black holes and wormholes: Quasinormal modes, ergoregion instability, and superradiance
We study scalar test-field perturbations on top of a Kerr–black-bounce background, ie, a
family of rotating regular black holes and/or rotating traversable wormholes that can mimic …
family of rotating regular black holes and/or rotating traversable wormholes that can mimic …
Stable rotating regular black holes
We present a rotating regular black hole whose inner horizon has zero surface gravity for
any value of the spin parameter and is, therefore, stable against mass inflation. Our metric is …
any value of the spin parameter and is, therefore, stable against mass inflation. Our metric is …
A connection between regular black holes and horizonless ultracompact stars
A bstract We illustrate that regular black holes and horizonless stars, typically considered as
quite distinct families of black hole mimickers, are intimately intertwined. We show that any …
quite distinct families of black hole mimickers, are intimately intertwined. We show that any …