Quasitopological Lifshitz black holes
- 1. Department of Physics and Engineering Physics, University of Saskatchewan, 116 Science Place, Saskatoon, Saskatchewan S7N 5E2 (Canada)
- 2. Department of Physics and Astronomy, University of Waterloo, 200 University Avenue West, Waterloo, Ontario, N2L 3G1 (Canada)
- 3. Research Institute for Astrophysics and Astronomy of Maragha (RIAAM), Maragha (Iran, Islamic Republic of)
- 4. Physics Department and Biruni Observatory, College of Sciences, Shiraz University, Shiraz 71454 (Iran, Islamic Republic of)
Description
We investigate the effects of including a quasitopological cubic curvature term to the Gauss-Bonnet action to five-dimensional Einstein gravity coupled to a Proca field and search for solutions with asymptotically Lifshitz scaling symmetry. We find that a new set of Lifshitz black hole solutions exist that are analogous to those obtained in third-order Lovelock gravity in higher dimensions. No additional matter fields are required to obtain solutions with asymptotic Lifshitz behavior, though we also investigate solutions with matter. Furthermore, we examine black hole solutions and their thermodynamics in this situation and find that a negative quasitopological term, just like a positive Gauss-Bonnet term, prevents instabilities in what are ordinarily unstable Einsteinian black holes.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.84.024012;
- arXiv
- arXiv:1101.3476v1;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 84
- Journal Issue
- 2
- Journal Page Range
- p. 024012-024012.12
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43079505
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ASYMPTOTIC SOLUTIONS; BLACK HOLES; GRAVITATION; INSTABILITY; SIMULATION; SYMMETRY; THERMODYNAMICS
- Descriptors DEC
- MATHEMATICAL SOLUTIONS
Optional Information
- Notes
- (c) 2011 American Institute of Physics