No-go theorems for hairy black holes in scalar- or vector-tensor-Gauss–Bonnet theory
DOI10.1088/1361-6382/ace94ezbMath1519.83058arXiv2210.03966OpenAlexW4384926705WikidataQ122271719 ScholiaQ122271719MaRDI QIDQ6116422
Publication date: 11 August 2023
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2210.03966
Vector fields, frame fields in differential topology (57R25) Black holes (83C57) Applications of Lie groups to the sciences; explicit representations (22E70) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Dirichlet series, exponential series and other series in one complex variable (30B50) Equations of motion in general relativity and gravitational theory (83C10) Matrix models and tensor models for quantum field theory (81T32)
Cites Work
- Black holes with only one Killing field
- Regular and black hole solutions of Einstein-Yang-Mills dilaton theory
- Analytic and asymptotically flat hairy (ultra-compact) black-hole solutions and their axial perturbations
- Black holes with synchronised Proca hair: linear clouds and fundamental non-linear solutions
- Black-Hole No-Hair Theorems for a Positive Cosmological Constant
- Do collapsed boson stars result in new types of black holes?
- Colored black holes
- A simple proof of a no-hair theorem in Einstein-Higgs theory
- First-order thermodynamics of scalar-tensor cosmology
- Spontaneous scalarisation of charged black holes: coupling dependence and dynamical features
- Kerr black holes with synchronised Proca hair: lensing, shadows and EHT constraints
- Past-directed scalar field gradients and scalar-tensor thermodynamics
This page was built for publication: No-go theorems for hairy black holes in scalar- or vector-tensor-Gauss–Bonnet theory
