RT Journal Article
T1 Sequences of extremal radially excited rotating black holes
A1 Blázquez Salcedo, José Luis
A1 Kunz, Jutta
A1 Navarro Lerida, Francisco
A1 Radu, Eugen
AB In the Einstein-Maxwell-Chern-Simons theory the extremal Reissner-Nordstrom solution is no longer the single extremal solution with vanishing angular momentum, when the Chern-Simons coupling constant reaches a critical value. Instead a whole sequence of rotating extremal J = 0 solutions arises, labeled by the node number of the magnetic U(1) potential. Associated with the same near horizon solution, the mass of these radially excited extremal solutions converges to the mass of the extremal Reissner-Nordstrom solution. On the other hand, not all near horizon solutions are also realized as global solutions.
PB American Physical Society
SN 0031-9007
YR 2014
FD 2014-01-10
LK https://hdl.handle.net/20.500.14352/98644
UL https://hdl.handle.net/20.500.14352/98644
LA eng
NO Blázquez-Salcedo, Jose Luis, et al. «Sequences of Extremal Radially Excited Rotating Black Holes». Physical Review Letters, vol. 112, n.o 1, enero de 2014, p. 011101. DOI.org (Crossref), https://doi.org/10.1103/PhysRevLett.112.011101.
NO Instituto de Salud Carlos III
NO German Research Foundation
NO Universidad Comlutense de Madrid
DS Docta Complutense
RD 8 abr 2025