First-order self-force analytic result for the total radiated energy of a radial infall from rest in Schwarzschild spacetime, for scalar and gravitational cases.
Gravitational field of a particle falling in a schwarzschild geometry analyzed in ten- sor harmonics
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
fields
gr-qc 3roles
background 1polarities
background 1representative citing papers
Pseudospectrum of Schwarzschild QNMs shows stability of the fundamental mode to infrared perturbations respecting asymptotics and instability of overtones to ultraviolet high-frequency perturbations.
Proves rigorous O(L^{-2}) localization estimates for resonance spectra in a compactly supported transfer-function model of black-hole echoes with explicit normalizations.
citing papers explorer
-
Analytic self-force effects on radial infalling particles in the Schwarzschild spacetime: the radiated energy
First-order self-force analytic result for the total radiated energy of a radial infall from rest in Schwarzschild spacetime, for scalar and gravitational cases.
-
Pseudospectrum and black hole quasi-normal mode (in)stability
Pseudospectrum of Schwarzschild QNMs shows stability of the fundamental mode to infrared perturbations respecting asymptotics and instability of overtones to ultraviolet high-frequency perturbations.
-
Black-Hole Echo Resonance Spectra and Source Dependence in a Controlled Transfer-Function Model
Proves rigorous O(L^{-2}) localization estimates for resonance spectra in a compactly supported transfer-function model of black-hole echoes with explicit normalizations.