The scattering map on collapsing charged spherically symmetric spacetimes
From MaRDI portal
Publication:6153393
DOI10.1088/1361-6382/ad259aarXiv2309.03025OpenAlexW4391464661MaRDI QIDQ6153393
Publication date: 19 March 2024
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2309.03025
Cites Work
- Unnamed Item
- Unnamed Item
- Time-translation invariance of scattering maps and blue-shift instabilities on Kerr black hole spacetimes
- Particle creation by black holes
- The charged dust solution of Ruban: Matching to Reissner-Nordström and shell crossings
- Scattering of scalar fields by spherical gravitational collapse
- The Hawking effect for spin 1/2 fields
- The \(r^{p}\)-weighted energy method of Dafermos and Rodnianski in general asymptotically flat spacetimes and applications
- Radiating shear-free gravitational collapse with charge
- The scattering map on Oppenheimer-Snyder space-time
- A non-degenerate scattering theory for the wave equation on extremal Reissner-Nordström
- A scattering theory for linear waves on the interior of Reissner-Nordström black holes
- Some Mathematical Aspects of the Hawking Effect for Rotating Black Holes
- A new physical-space approach to decay for the wave equation with applications to black hole spacetimes
- The red‐shift effect and radiation decay on black hole spacetimes
- A new uniqueness theorem for charged black holes
- L'effet Hawking
- Lectures on black holes and linear waves
- On Continued Gravitational Contraction
- Complétude asymptotique pour l'équation des ondes dans une classe d'espaces-temps stationnaires et asymptotiquement plats. (Asymptotic completeness for the wave equation in a class of stationary and asymptotically flat space-times)
This page was built for publication: The scattering map on collapsing charged spherically symmetric spacetimes
