Quantizing dust geodesics in a generalized Kerr metric gives a rotating black-hole core that is smaller and equator-elongated relative to the spherical case, with a linear mass/angular-momentum interior profile that avoids Cauchy horizons.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
gr-qc 2representative citing papers
Reviews quantum dust core black hole model with linear Misner-Sharp-Hernandez mass function and computes its quasi-normal modes, showing deviations from Schwarzschild sensitive to core surface quantum properties.
citing papers explorer
-
Quantum dust cores of rotating black holes
Quantizing dust geodesics in a generalized Kerr metric gives a rotating black-hole core that is smaller and equator-elongated relative to the spherical case, with a linear mass/angular-momentum interior profile that avoids Cauchy horizons.
-
Quantum dust cores of black holes and their quasi-normal modes
Reviews quantum dust core black hole model with linear Misner-Sharp-Hernandez mass function and computes its quasi-normal modes, showing deviations from Schwarzschild sensitive to core surface quantum properties.