An RG-improved Schwarzschild metric with de Sitter core is studied for shadow radius, scalar/EM/Dirac quasinormal modes via WKB and time-domain methods, SCC compliance at the inner horizon, and a Davies-type thermodynamic phase transition.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
fields
gr-qc 2years
2026 2verdicts
UNVERDICTED 2roles
background 1polarities
background 1representative citing papers
Dark matter halos suppress Hawking temperature and emission rates in regular black holes while enabling a range of horizon radii with positive specific heat capacity and a Davies-type phase transition.
citing papers explorer
-
Renormalization-group improved Schwarzschild black hole: shadow, ringdown, and strong cosmic censorship
An RG-improved Schwarzschild metric with de Sitter core is studied for shadow radius, scalar/EM/Dirac quasinormal modes via WKB and time-domain methods, SCC compliance at the inner horizon, and a Davies-type thermodynamic phase transition.
-
Hawking Temperature, Sparsity and Energy Emission Rate of Dark Matter Halo Regular Black Holes
Dark matter halos suppress Hawking temperature and emission rates in regular black holes while enabling a range of horizon radii with positive specific heat capacity and a Davies-type phase transition.