- Access by Xinjiang University
Spin-3 quasinormal modes of the BTZ black hole
Phys. Rev. D 85, 084007 – Published 6 April, 2012
DOI: https://doi.org/10.1103/PhysRevD.85.084007
Abstract
Using the operator approach, we obtain quasinormal modes (QNMs) of the Bañados-Teitelboim-Zanelli black hole in spin-3 topologically massive gravity by solving the first-order equation of motion with the transverse-traceless condition. We find that these are different from those obtained when solving the second-order differential equation for the third-rank tensor of spin-3 field subject to suitable boundary conditions and having the sign ambiguity of mass. However, it is shown clearly that two approaches to the left-moving QNMs are identical, while the right-moving QNMs of solving the second-order equation are given by descendants of the operator approach.
Article Text
References (10)
- M. Henneaux and S.-J. Rey, J. High Energy Phys. 12 (2010) 007.
- A. Campoleoni, S. Fredenhagen, S. Pfenninger,and S. Theisen, J. High Energy Phys. 11 (2010) 007.
- B. Chen, J. Long,and J. b. Wu, Phys. Lett. B 705, 513 (2011).
- A. Bagchi, S. Lal, A. Saha, and B. Sahoo, J. High Energy Phys. 10 (2011) 150.
- W. Li, W. Song, and A. Strominger, J. High Energy Phys. 04 (2008) 082.
- S. Datta and J. R. David, J. High Energy Phys. 03 (2012) 079.
- I. Sachs and S. N. Solodukhin, J. High Energy Phys. 08 (2008) 003.
- Y. S. Myung, Y. W. Kim, T. Moon, and Y. J. Park, Phys. Rev. D 84, 024044 (2011).
- D. Birmingham, S. Mokhtari, and I. Sachs, Phys. Rev. D 82, 124059 (2010).
- I. Sachs, J. High Energy Phys. 09 (2008) 073.