Hairy black hole solutions in \(U(1)\) gauge-invariant scalar-vector-tensor theories

DOI10.1016/j.physletb.2018.03.059zbMath1390.83204arXiv1802.07035OpenAlexW2788774649MaRDI QIDQ1750608

Lavinia Heisenberg, Shinji Tsujikawa

Publication date: 22 May 2018

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1802.07035

Mathematics Subject Classification ID

Black holes (83C57) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items (7)

Spin-orbit effects for compact binaries in scalar-tensor gravity ⋮ Scalar fields near compact objects: resummation versus UV completion ⋮ Inflation in a scalar-vector-tensor theory ⋮ Inflation driven by massive vector fields with derivative self-interactions ⋮ Superradiant instability and asymptotically AdS hairy black holes in \(F(R)\)-charged scalar field theory ⋮ Scalar-vector-tensor gravity theories ⋮ Dark energy in scalar-vector-tensor theories

Cites Work

• Derivative self-interactions for a massive vector field
• Scalar hair from a derivative coupling of a scalar field to the Einstein tensor
• Black holes and neutron stars in vector Galileons

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