### Abstract

In this work, we compute the conserved quantities of a charged rotating black hole which appears as the solution of Einstein-Maxwell action in five dimensions coupled to a Chern-Simons term for U(1) field. The addition of the Chern-Simons term will modify the Maxwell equations and the definition of charge but not the Einstein field equations. Upon the addition of suitable boundary terms for the pure gravity sector of the theory, which depend on the extrinsic and intrinsic curvatures (Kounterterms), we obtain the correct conserved quantities of the solution.

Original language | English |
---|---|

Article number | 012022 |

Journal | Journal of Physics: Conference Series |

Volume | 1043 |

Issue number | 1 |

DOIs | |

Publication status | Published - 25 Jun 2018 |

Event | 20th Chilean Physics Symposium - Santiago, Chile Duration: 30 Nov 2016 → 2 Dec 2016 |

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### ASJC Scopus subject areas

- Physics and Astronomy(all)

### Cite this

*Journal of Physics: Conference Series*,

*1043*(1), [012022]. https://doi.org/10.1088/1742-6596/1043/1/012022

}

*Journal of Physics: Conference Series*, vol. 1043, no. 1, 012022. https://doi.org/10.1088/1742-6596/1043/1/012022

**Conserved quantities for a charged rotating black holes in 5D Einstein-Maxwell-Chern-Simons theory.** / Diaz-Martinez, Felipe; Olea, Rodrigo.

Research output: Contribution to journal › Conference article

TY - JOUR

T1 - Conserved quantities for a charged rotating black holes in 5D Einstein-Maxwell-Chern-Simons theory

AU - Diaz-Martinez, Felipe

AU - Olea, Rodrigo

PY - 2018/6/25

Y1 - 2018/6/25

N2 - In this work, we compute the conserved quantities of a charged rotating black hole which appears as the solution of Einstein-Maxwell action in five dimensions coupled to a Chern-Simons term for U(1) field. The addition of the Chern-Simons term will modify the Maxwell equations and the definition of charge but not the Einstein field equations. Upon the addition of suitable boundary terms for the pure gravity sector of the theory, which depend on the extrinsic and intrinsic curvatures (Kounterterms), we obtain the correct conserved quantities of the solution.

AB - In this work, we compute the conserved quantities of a charged rotating black hole which appears as the solution of Einstein-Maxwell action in five dimensions coupled to a Chern-Simons term for U(1) field. The addition of the Chern-Simons term will modify the Maxwell equations and the definition of charge but not the Einstein field equations. Upon the addition of suitable boundary terms for the pure gravity sector of the theory, which depend on the extrinsic and intrinsic curvatures (Kounterterms), we obtain the correct conserved quantities of the solution.

UR - http://www.scopus.com/inward/record.url?scp=85050144695&partnerID=8YFLogxK

U2 - 10.1088/1742-6596/1043/1/012022

DO - 10.1088/1742-6596/1043/1/012022

M3 - Conference article

VL - 1043

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

SN - 1742-6588

IS - 1

M1 - 012022

ER -