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    LNRF-velocity hump-induced oscillations of a Keplerian disc orbiting near-extreme Kerr black hole: a possible explanation of high-frequency QPOs in GRS 1915+105

    Zdeněk Stuchlík · Srpen 01, 2007 · Fyzika · 0 comments
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    Publication date: Aug 2007

    Abstract:
    Context: At least four high-frequency quasiperiodic oscillations (QPOs)
    at frequencies 41 Hz, 67 Hz, 113 Hz, and 167 Hz were reported in a
    binary system GRS 1915+105 hosting near-extreme Kerr black hole with a
    dimensionless spin a > 0.98.
    Aims: We attempt to explain all
    four observed frequencies by an extension of the standard resonant model
    of epicyclic oscillations.
    Methods: We use the idea of
    oscillations induced by the hump of the orbital velocity profile
    (related to locally non-rotating frames-LNRF) in discs orbiting near-
    extreme Kerr black holes, which are characterized by a “humpy frequency”
    ν_h, that could excite the radial and vertical epicyclic oscillations
    with frequencies ν_r, ν_v. Due to non-linear resonant phenomena, the
    combinational frequencies are allowed as well.
    Results: Assuming
    mass M = 14.8 M☉ and spin a = 0.9998 for the GRS 1915+105
    Kerr black hole, the model predicts frequencies νh = 41 Hz,
    νr = 67 Hz, ν_h+νr = 108 Hz, and ν_v-νr
    = 170 Hz corresponding quite well to the observed ones.
    Conclusions: For black-hole parameters being in good agreement with
    those given observationally, the forced resonant phenomena in non-linear
    oscillations, excited by the “hump-induced” oscillations in a Keplerian
    disc, can explain high-frequency QPOs in near-extreme Kerr black-hole
    binary system GRS 1915+105 within the range of observational errors.

    Authors:
    Stuchlík, Z.; Slaný, P.; Török, G.;

    https://ui.adsabs.harvard.edu/abs/2007A&A…470..401S

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