Primordial Black Hole Evolution in Tensor-Scalar Cosmology
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Publication:4492626
DOI10.1103/PhysRevLett.83.2699zbMath0951.83029arXivastro-ph/9905303OpenAlexW1991950525MaRDI QIDQ4492626
Publication date: 16 July 2000
Published in: Physical Review Letters (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/astro-ph/9905303
Relativistic cosmology (83F05) Black holes (83C57) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
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Black hole hair from scalar dark matter ⋮ Vortex hair on AdS black holes ⋮ Spin-orbit effects for compact binaries in scalar-tensor gravity ⋮ Black holes and scalar fields ⋮ Observable effects of scalar fields and varying constants ⋮ Unveiling the Galileon in a three-body system: scalar and gravitational wave production ⋮ Gravitational couplings in Chameleon models ⋮ Extreme mass ratio inspirals with scalar hair ⋮ Extreme gravity tests with gravitational waves from compact binary coalescences. I: Inspiral-merger ⋮ A tachyon field around the black hole ⋮ Quantum‐corrected Geometry of Horizon Vicinity ⋮ Non-singular Brans-Dicke collapse in deformed phase space ⋮ Building cosmological frozen stars ⋮ Black hole thermodynamics with dynamical lambda ⋮ Hawking radiation from cubic and quartic black holes via tunneling of GUP corrected scalar and fermion particles ⋮ Effective field theory of black hole quasinormal modes in scalar-tensor theories ⋮ Cylindrical systems in general relativity ⋮ Quasilocal mass in scalar–tensor gravity: spherical symmetry ⋮ Quasilocal energy in modified gravity ⋮ The confrontation between general relativity and experiment ⋮ Gauge independent response of a laser interferometer to gravitational waves ⋮ Evolving black holes in inflation ⋮ Ladder symmetries of black holes. Implications for love numbers and no-hair theorems ⋮ ACCRETION OF NONMINIMALLY COUPLED GENERALIZED CHAPLYGIN GAS INTO BLACK HOLES ⋮ Vortices and waves in light dark matter ⋮ Static response and Love numbers of Schwarzschild black holes
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