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Black hole accretion discs and screened scalar hair

We present a novel way to investigate scalar field profiles around black holes with an accretion disc for a range of models where the Compton wavelength of the scalar is large compared to other length scales. By analysing the problem in "Weyl" coordinates, we are able to calculate the scalar profiles for accretion discs in the static Schwarzschild, as well as rotating Kerr, black holes. We comment on observational effects.

preprint2016arXivOpen access
Anne-Christine DavisRuth GregoryRahul Jha
astro-ph.COgr-qchep-th
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Anne-Christine DavisRuth GregoryRahul Jha

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