ADVANCED METHODS IN BLACK-HOLE PERTURBATION THEORY

DOI10.1142/S0217751X13400186zbMath1277.83054arXiv1305.6759OpenAlexW3105414620MaRDI QIDQ2866875

Paolo Pani

Publication date: 9 December 2013

Published in: International Journal of Modern Physics A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1305.6759

zbMATH Keywords

perturbation theorynumerical methodsblack holesgravitational waves

Mathematics Subject Classification ID

Black holes (83C57) Perturbations in context of PDEs (35B20) Gravitational waves (83C35)

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Cites Work

• Unnamed Item
• Unnamed Item
• Quasi-normal modes and gravitational wave astronomy
• Instability of black holes in massive gravity
• INITIAL CONDITIONS FOR NUMERICAL RELATIVITY: INTRODUCTION TO NUMERICAL METHODS FOR SOLVING ELLIPTIC PDEs
• NUMERICAL RELATIVITY IN HIGHER-DIMENSIONAL SPACE–TIMES
• Numerical investigation of the late-time Kerr tails
• On the non-radial oscillations of slowly rotating stars induced by the Lense-Thirring effect
• Quasinormal modes of black holes and black branes
• Lectures on holographic methods for condensed matter physics
• Spectral Methods in MATLAB
• Gravitational quasinormal modes for anti-de Sitter black holes
• Bosenova Collapse of Axion Cloud around a Rotating Black Hole
• Tidal acceleration of black holes and superradiance
• Quasinormal modes: the characteristic `sound' of black holes and neutron stars
• Black holes in higher dimensions