On the motion of hairy black holes in Einstein-Maxwell-dilaton theories

DOI10.1088/1475-7516/2018/01/026OpenAlexW3105289532MaRDI QIDQ5021787

Félix-Louis Julié

Publication date: 14 January 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1711.10769

zbMATH Keywords

modified gravitygravitational waves/theorygravitational waves/sources

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (10)

Minimal spin deflection of Kerr-Newman and supersymmetric black hole ⋮ Scalar charges and the first law of black hole thermodynamics ⋮ Bianchi IX geometry and the Einstein–Maxwell theory ⋮ Extreme mass ratio inspirals with scalar hair ⋮ Time evolution of Einstein-Maxwell-scalar black holes after a thermal quench ⋮ Schwarzschild-like topological solitons ⋮ Gravitational waves from eccentric extreme mass-ratio inspirals as probes of scalar fields ⋮ Smooth bubbling geometries without supersymmetry ⋮ Post-Newtonian gravitational and scalar waves in scalar-Gauss–Bonnet gravity ⋮ Gravitational radiation from compact binary systems in Einstein-Maxwell-dilaton theories

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• Moduli space metric for maximally-charged dilaton black holes
• Interparticle potential up to next-to-leading order for gravitational, electrical, and dilatonic forces
• Tensor-multi-scalar theories of gravitation
• Multicentered solution for maximally charged dilaton black holes in arbitrary dimensions
• Gravitational radiation from post-Newtonian sources and inspiralling compact binaries

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