Magnetic and electric black holes in arbitrary dimensions
Creators
- 1. Centre National de l'Energie, des Sciences et des Techniques Nucleaires, CNESTEN, Cellule Sciences de la Matiere, Rabat, Morocco and Groupement National de Physique des Hautes Energies, GNPHE, Siege focal: FS, Rabat (Morocco)
- 2. Departamento de Fisica Teorica, Universidad de Zaragoza, Pedro Cerbuna, 12. E-50009 Zaragoza (Spain)
Description
In this work, we compare two different objects: electric black holes and magnetic black holes in arbitrary dimension. The comparison is made in terms of the corresponding moduli space and their extremal geometries. We treat parallelly the magnetic and the electric cases. Specifically, we discuss the gravitational solution of these spherically symmetric objects in the presence of a positive cosmological constant. Then, we find the bounded region of the moduli space allowing the existence of black holes. After identifying it in both the electric and the magnetic case, we calculate the geometry that comes out between the horizons at the coalescence points. Although the electric and magnetic cases are both very different (only dual in four dimensions), gravity solutions seem to clear up most of the differences and lead to very similar geometries.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.80.044015;
- arXiv
- arXiv:0906.0489v1;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 80
- Journal Issue
- 4
- Journal Page Range
- p. 044015-044015.9
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41063597
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- BLACK HOLES; COALESCENCE; COMPARATIVE EVALUATIONS; COMPUTERIZED SIMULATION; COSMOLOGICAL CONSTANT; GRAVITATION; GRAVITATIONAL WAVES; MATHEMATICAL SOLUTIONS; SPACE; SYMMETRY
- Descriptors DEC
- EVALUATION; SIMULATION
Optional Information
- Notes
- (c) 2009 The American Physical Society