Scalar, electromagnetic and Weyl perturbations of BTZ black holes: Quasinormal modes

By V. Cardoso, J. Lemos. 2001

321 citations recorded by the source corpus.

We calculate the quasinormal modes and associated frequencies of the Banados-Teitelboim-Zanelli (BTZ) nonrotating black hole. This black hole lives in 2+1 dimensions in an asymptotically anti{endash}de Sitter spacetime. We obtain exact results for the wave function and quasinormal frequencies of scalar, electromagnetic and Weyl (neutrino) perturbations.

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

View Paper: https://www.semanticscholar.org/paper/dcdbca1f8e3940175bafb5ab3d981bb660221bae

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. S. Sachdev
2. S. Hartnoll
3. Frederik Denef
4. Alvaro Núñez
5. A. Starinets
6. G. Horowitz
7. Andrew Lucas
8. R. Myers

In Nuclear and High Energy Physics

1. S. Hartnoll
2. S. Sachdev
3. Frederik Denef
4. Christopher P. Herzog
5. G. Horowitz
6. Alvaro Núñez
7. A. Starinets
8. S. Gubser

In Statistical and Nonlinear Physics

1. S. Sachdev
2. S. Hartnoll
3. Frederik Denef
4. A. Starinets
5. Alvaro Núñez
6. Christopher P. Herzog
7. S. Gubser
8. G. Horowitz

Citations in the corpus

• AdS / CFT correspondence, quasinormal modes, and thermal correlators in N=4 SYM (2003, background): “22) bears resemblance to spectra of scalar quasinormal frequencies of the two asymptotically AdS backgrounds where the modes can be found exactly, the (2 + 1)-dimensional BTZ black hole [20],[19], [21] and the 4d massless topological black hole [27].”
• Black hole determinants and quasinormal modes (2009, background): “The quasinormal frequencies of a neutral massive scalar of mass m2 = ∆(∆ − 1)/L2 in a nonrotating BTZ black hole background are [55, 29, 16] zp,s,± = ± p L − 2πT i(∆ + 2s) , s = 0, 1, 2, .”