Quasinormal modes of Schwarzschild anti-de Sitter black holes: Electromagnetic and gravitational perturbations

By V. Cardoso, J. Lemos. 2001

308 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/3653701d856dfe0634c55ca762f77e1218e9137b

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. V. Cardoso
2. Paolo Pani
3. R. Brito
4. A. Starinets
5. Jorge E Santos
6. Gavin Hartnett
7. Ó. J. Dias
8. S. Hartnoll

In Nuclear and High Energy Physics

1. V. Cardoso
2. Paolo Pani
3. R. Brito
4. A. Starinets
5. Jorge E Santos
6. S. Hartnoll
7. Ó. J. Dias
8. D. Son

In Statistical and Nonlinear Physics

1. A. Starinets
2. S. Hartnoll
3. V. Cardoso
4. D. Son
5. R. Schiappa
6. José Natário
7. Jorge E Santos
8. Ó. J. Dias

Citations in the corpus

• Quasinormal modes of near extremal black branes (2002, background): “3) in the Regge- Wheeler form and essentially repeating the proofs for AdS black holes given recently in [12], [13].”
• An Analytical computation of asymptotic Schwarzschild quasinormal frequencies (2002, background): “The recurrence relation describing the quasinormal modes of AdS black holes has also been studied [30, 31, 32].”
• Holographic thermalization, quasinormal modes and superradiance in Kerr-AdS (2013, methodology): “The associated QNMs of the global AdS Schwarzchild BH were then computed [9, 10, 30]: vector QNMs agree with those first computed in [31, 32, 33] (the scalar modes of [31, 32, 33] do not preserve the asymptotic AdS structure).”
• On the classification of asymptotic quasinormal frequencies for $d$-dimensional black holes and quantum gravity (2004, background): “Quasinormal modes of Schwarzschild AdS black holes were first addressed in [57, 58, 59, 60] although the emphasis lied in the lowest frequency modes (with [60] focusing on spinor perturbations).”
• Superradiance (2015, result): “For both scalar and vector modes the imaginary part of the frequency is negative at a = 0, consistent with the fact that QNMs of Schwarzschild-AdS are always damped [54, 392].”
• Minkowski-space correlators in AdS/CFT correspondence: recipe and applications (2002, background): “ and references on quasinormal modes in asymptotically flat spacetimes see [16, 17]. 3Similar ideas appear in ref. [19]. Other works on quasinormal modes in asymptotically AdS spacetimes include refs. [20, 21, 22, 23, 24]. – 16 – 5. Thermal N = 4 SYM theory and the Chern-Simons diffusion rate We now c”
• Superradiance: Energy Extraction, Black-Hole Bombs and Implications for Astrophysics and Particle Physics (2015, result): “For both scalar and vector modes the imaginary part of the frequency is negative at a = 0, consistent with the fact that QNMs of Schwarzschild-AdS are always damped [51, 306].”