For Poisson-sprinkled causal sets in 1+1D Minkowski space, the averaged massless retarded propagator is a normalized exp(L) with L the link matrix; the massive case via mass-scattering series agrees with the continuum after averaging.
Title resolution pending
8 Pith papers cite this work. Polarity classification is still indexing.
8
Pith papers citing it
years
2026 8representative citing papers
Vaidya-type dynamical black holes admit homothetic Killing vectors only for linear-in-null-time mass/charge/rotation profiles, and the resulting homothetic Killing horizons carry surface gravities obeying a flux-balance first law.
Effective field theory yields model-independent corrections to Kerr black hole quasinormal modes that oscillate logarithmically near extremality, indicating discrete scale invariance.
Bosonic nonlocal correlations degrade at finite radial distances from the event horizon and vanish at larger distances when the quantum atmosphere is accounted for, showing stronger response than in fermionic cases.
Tsallis and Barrow non-extensive entropy corrections modify the thermodynamic stability, phase transitions, and Joule-Thomson cooling behavior of deformed AdS-Schwarzschild 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.
Derives static spherically symmetric black hole metric combining ModMax electrodynamics, Lorentz-violating Kalb-Ramond gravity, and perfect-fluid dark matter, then analyzes thermodynamic quantities and stability.
The authors calculate horizons, Hawking temperature, heat capacity, effective potentials, epicyclic frequencies, and shadows for a GR+NED+PFDM black hole, then constrain mass, magnetic charge, PFDM parameter, and orbital radius via MCMC on QPO observations from XTE J1550-564 and similar sources.
citing papers explorer
-
Link-based causal set propagators in $1+1$ dimensions
For Poisson-sprinkled causal sets in 1+1D Minkowski space, the averaged massless retarded propagator is a normalized exp(L) with L the link matrix; the massive case via mass-scattering series agrees with the continuum after averaging.
-
Homothetic Killing horizons in generic Vaidya spacetimes
Vaidya-type dynamical black holes admit homothetic Killing vectors only for linear-in-null-time mass/charge/rotation profiles, and the resulting homothetic Killing horizons carry surface gravities obeying a flux-balance first law.
-
Kerr Black Hole Ringdown in Effective Field Theory
Effective field theory yields model-independent corrections to Kerr black hole quasinormal modes that oscillate logarithmically near extremality, indicating discrete scale invariance.
-
Nonlocal correlations for bosonic fields in black hole quantum atmosphere
Bosonic nonlocal correlations degrade at finite radial distances from the event horizon and vanish at larger distances when the quantum atmosphere is accounted for, showing stronger response than in fermionic cases.
-
Thermodynamics of Deformed AdS-Schwarzschild Black Holes Beyond the Bekenstein Paradigm
Tsallis and Barrow non-extensive entropy corrections modify the thermodynamic stability, phase transitions, and Joule-Thomson cooling behavior of deformed AdS-Schwarzschild black holes.
-
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.
-
ModMax black hole surrounded by perfect-fluid dark matter in Lorentz-violating Kalb-Ramond gravity
Derives static spherically symmetric black hole metric combining ModMax electrodynamics, Lorentz-violating Kalb-Ramond gravity, and perfect-fluid dark matter, then analyzes thermodynamic quantities and stability.
-
Black holes in general relativity coupled with NEDs surrounded by PFDM: thermodynamics, epicyclic oscillations, QPOs, and shadow
The authors calculate horizons, Hawking temperature, heat capacity, effective potentials, epicyclic frequencies, and shadows for a GR+NED+PFDM black hole, then constrain mass, magnetic charge, PFDM parameter, and orbital radius via MCMC on QPO observations from XTE J1550-564 and similar sources.