RT Journal Article
T1 Angular momentum – area – proportionality of extremal charged black holes in odd dimensions
A1 Blázquez Salcedo, José Luis
A1 Kunz, Jutta
A1 Navarro Lerida, Francisco
AB Extremal rotating cohomogeneity-1 black holes in Einstein-Maxwell theory feature two branches. On the branch emerging from the Myers-Perry solutions their angular momentum is proportional to their horizon area, while on the branch emerging from the Tangherlini solutions their angular momentum is proportional to their horizon angular momentum. The transition between these branches occurs at a critical value of the charge, which depends on the value of the angular momentum. However, when a dilaton is included, the angular momentum is always proportional to the horizon area.
PB Elsevier
SN 0370-2693
YR 2013
FD 2013-11-25
LK https://hdl.handle.net/20.500.14352/98615
UL https://hdl.handle.net/20.500.14352/98615
LA eng
NO Blázquez-Salcedo, Jose Luis, et al. «Angular Momentum – Area – Proportionality of Extremal Charged Black Holes in Odd Dimensions». Physics Letters B, vol. 727, n.o 1-3, noviembre de 2013, pp. 340-44. DOI.org (Crossref), https://doi.org/10.1016/j.physletb.2013.10.046.
NO Instituto de Salud Carlos III
NO German Research Foundation
NO Universidad Comlutense de Madrid
DS Docta Complutense
RD 20 abr 2025