Black holes with synchronised Proca hair: linear clouds and fundamental non-linear solutions

DOI10.1007/JHEP07(2020)010zbMath1475.83045arXiv2004.09536OpenAlexW3104800817MaRDI QIDQ2215319

Luís C. B. Crispino, Eugen Radu, Nuno M. Santos, Carolina L. Benone, Carlos A. R. Herdeiro

Publication date: 11 December 2020

Published in: Journal of High Energy Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2004.09536

zbMATH Keywords

black holesclassical theories of gravityProca star

Mathematics Subject Classification ID

Black holes (83C57) Methods of quantum field theory in general relativity and gravitational theory (83C47) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (8)

Kerr black holes with synchronised Proca hair: lensing, shadows and EHT constraints ⋮ Ultralight bosons for strong gravity applications from simple Standard Model extensions ⋮ Proca-Higgs balls and stars in a UV completion for Proca self-interactions ⋮ No-go theorems for hairy black holes in scalar- or vector-tensor-Gauss–Bonnet theory ⋮ Kaluza-Klein monopole with scalar hair ⋮ \(D = 5\) static, charged black holes, strings and rings with resonant, scalar \(Q\)-hair ⋮ Black holes, stationary clouds and magnetic fields ⋮ Analytic and asymptotically flat hairy (ultra-compact) black-hole solutions and their axial perturbations

Cites Work

• Unnamed Item
• Stationary scalar clouds around a BTZ black hole
• Massive vector fields in Kerr-Newman and Kerr-Sen black hole spacetimes
• Separation of Maxwell equations in Kerr-NUT-(A)dS spacetimes
• Spinning Kerr black holes with stationary massive scalar clouds: the large-coupling regime
• Maxwell's equations in the Myers-Perry geometry
• Gravitating solitons and black holes with synchronised hair in the four dimensional O(3) sigma-model
• Asymptotically flat spinning scalar, Dirac and Proca stars
• Kerr black holes with synchronised scalar hair and boson stars in the Einstein-Friedberg-Lee-Sirlin model
• Quasi-bound states of massive scalar fields in the Kerr black-hole spacetime: beyond the hydrogenic approximation
• Spherical null geodesics of rotating Kerr black holes
• Hamilton-Jacobi and Schrödinger separable solutions of Einstein's equations
• Black holes, hidden symmetries, and complete integrability
• Instability of charged massive scalar fields in bound states around Kerr–Sen black holes
• Asymptotically flat black holes with scalar hair: A review
• Kerr black holes with Proca hair
• Shadows of Kerr black holes with and without scalar hair
• Testing the black hole ‘no-hair’ hypothesis
• The large-mass limit of cloudy black holes
• Construction and physical properties of Kerr black holes with scalar hair
• Scalar clouds around Kerr–Sen black holes
• The spectra of gravitational atoms
• Stationary scalar clouds around maximally rotating linear dilaton black holes
• Global Structure of the Kerr Family of Gravitational Fields
• Théorie non relativiste des particules à spin entier

This page was built for publication: Black holes with synchronised Proca hair: linear clouds and fundamental non-linear solutions