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We present a family of exact black-hole solutions on a static spherically symmetric background in second-order generalized Proca theories with derivative vector-field interactions coupled to gravity. We also derive nonexact solutions in power-law coupling models including vector Galileons and numerically show the existence of regular black holes with a primary hair associated with the longitudinal propagation. The intrinsic vector-field derivative interactions generally give rise to a secondary hair induced by nontrivial field profiles. The deviation from General Relativity is most significant around the horizon and hence there is a golden opportunity for probing the Proca hair by the measurements of gravitational waves (GWs) in the regime of strong gravity.
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Lavinia Heisenberg
Heidelberg University
Ryotaro Kase
Tokyo University of Science
Masato Minamitsuji
Instituto de Engenharia de Sistemas e Computadores Investigação e Desenvolvimento
Physical review. D/Physical review. D.
ETH Zurich
University of Lisbon
Tokyo University of Science
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Heisenberg et al. (Tue,) studied this question.
synapsesocial.com/papers/6a204cb0284a522d2e2ed58a — DOI: https://doi.org/10.1103/physrevd.96.084049
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