pith. machine review for the scientific record. sign in

arxiv: 1711.03390 · v2 · submitted 2017-11-09 · ✦ hep-th · gr-qc

Recognition: unknown

Evasion of No-Hair Theorems and Novel Black-Hole Solutions in Gauss-Bonnet Theories

Authors on Pith no claims yet
classification ✦ hep-th gr-qc
keywords black-holesolutionscouplingeasilyno-hairregulartheoremstheory
0
0 comments X
read the original abstract

We consider a general Einstein-scalar-GB theory with a coupling function f(\phi). We demonstrate that black-hole solutions appear as a generic feature of this theory since a regular horizon and an asymptotically-flat solution may be easily constructed under mild assumptions for f(\phi). We show that the existing no-hair theorems are easily evaded, and a large number of regular, black-hole solutions with scalar hair are then presented for a plethora of coupling functions f(\phi).

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 10 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. No-go theorem for spontaneous vectorization

    gr-qc 2026-05 unverdicted novelty 8.0

    A no-go theorem shows that negative effective mass squared for the vector field in vector-tensor gravity always accompanies ghost or gradient instabilities, blocking spontaneous vectorization in stationary axisymmetri...

  2. Gravitational Memory from Hairy Binary Black Hole Mergers

    gr-qc 2026-04 unverdicted novelty 8.0

    Gravitational memory from hairy binary black hole mergers in scalar-Gauss-Bonnet gravity differs from GR by a few percent due to altered nonlinear dynamics, with direct scalar contributions suppressed, and including m...

  3. Inspiral gravitational waveforms from charged compact binaries with scalar hair

    gr-qc 2026-05 unverdicted novelty 7.0

    In Einstein-scalar-Maxwell theories, charged compact binaries produce gravitational waveforms containing a leading -1 post-Newtonian dipole correction controlled by one deviation parameter b.

  4. Spin-Induced Nonlinear Scalarization of Kerr Black Holes in Einstein-scalar-Gauss-Bonnet Gravity

    gr-qc 2026-04 unverdicted novelty 7.0

    Kerr black holes in an EsGB model without linear instability undergo nonlinear scalarization above spin 0.5, existing in a finite low-mass high-spin wedge rather than a narrow band.

  5. Phase transition structure of scalarized neutron stars: the effect of rotation and linear coupling

    gr-qc 2026-04 unverdicted novelty 6.0

    Linear coupling and rotation in scalar-tensor theories produce a complex phase transition landscape for scalarized neutron stars, with rotation increasing critical masses and Landau theory revealing overlooked solutio...

  6. Spin-charge induced scalarization of Kerr-Newman black holes in the Einstein-Maxwell-scalar theory with scalar potential

    gr-qc 2026-04 unverdicted novelty 6.0

    Kerr-Newman black holes in EMS theory with scalar potential scalarize for spins below a threshold set by charge, scalar mass, and coupling strength.

  7. On cosmological properties of black-hole hair in linearly coupled scalar-Gauss-Bonnet theory

    gr-qc 2026-05 unverdicted novelty 5.0

    Scalar hair sourced by black holes in de Sitter spacetime grows temporally and spatially on superhorizon scales due to the dynamics of a minimally coupled massless scalar field in expanding spacetime, carrying a stead...

  8. Regular hairy black holes by gravitational decoupling: Bardeen and Minkowski-core seeds

    gr-qc 2026-05 unverdicted novelty 5.0

    Two families of regular hairy black holes are generated from Bardeen and Minkowski-core seeds using gravitational decoupling with an exponential profile, yielding de Sitter or flat cores, critical horizon parameters, ...

  9. Minimum mass, maximum charge and hyperbolicity in scalar Gauss-Bonnet gravity

    gr-qc 2026-04 unverdicted novelty 5.0

    In scalar Gauss-Bonnet gravity, black hole solutions below a tunable minimum mass lose hyperbolicity in perturbations, corresponding to EFT breakdown, but scalar charge stays bounded above.

  10. Thermodynamics and phase transitions of nonlinearly scalarized black holes in Einstein-scalar-Gauss-Bonnet theory

    gr-qc 2026-04 unverdicted novelty 4.0

    Nonlinearly scalarized black holes in Einstein-scalar-Gauss-Bonnet theory undergo a first-order phase transition from Schwarzschild black holes with non-zero latent heat.