Hydrodynamical response of a circumbinary gas disc to black hole recoil and mass loss

Lia R. Corrales, Zoltán Haiman, Andrew MacFadyen

    Research output: Contribution to journalArticle

    Abstract

    Finding electromagnetic (EM) counterparts of future gravitational wave (GW) sources would bring rich scientific benefits. A promising possibility, in the case of the coalescence of a supermassive black hole binary (SMBHB), is that the prompt emission from merger-induced disturbances in a supersonic circumbinary disc may be detectable. We follow the post-merger evolution of a thin, zero-viscosity circumbinary gas disc with two-dimensional simulations, using the hydrodynamic code flash. We analyse perturbations arising from the 530 km s-1 recoil of a 106 M binary, oriented in the plane of the disc, assuming either a non-radiative gamma-law or a pseudo-isothermal equation of state for the gas. We find that a single-armed spiral shock wave forms and propagates outwards, sweeping up ∼40 per cent of the mass of the disc. The morphology and evolution of the perturbations agrees well with those of caustics predicted to occur in a collisionless disc. Assuming that the disc radiates nearly instantaneously to maintain a constant temperature, we estimate the amount of dissipation and corresponding post-merger light curve. The luminosity rises steadily on the time-scale of months, and reaches few ×1043 erg s-1, corresponding to ≈10 per cent of the Eddington luminosity of the central SMBHB. We also analyse the case in which gravitational wave emission results in a 5 per cent mass loss in the merger remnant. The mass loss reduces the shock overdensities and the overall luminosity of the disc by ≈15-20 per cent, without any other major effects on the spiral shock pattern.

    Original languageEnglish (US)
    Pages (from-to)947-962
    Number of pages16
    JournalMonthly Notices of the Royal Astronomical Society
    Volume404
    Issue number2
    DOIs
    StatePublished - May 2010

    Fingerprint

    merger
    gases
    gas
    perturbation
    luminosity
    gravitational waves
    coalescence
    shock wave
    equation of state
    erg
    shock
    gas viscosity
    dissipation
    viscosity
    hydrodynamics
    timescale
    disturbance
    loss
    coalescing
    light curve

    Keywords

    • Black hole physics
    • Galaxies: nuclei
    • Gravitational waves

    ASJC Scopus subject areas

    • Space and Planetary Science
    • Astronomy and Astrophysics

    Cite this

    Hydrodynamical response of a circumbinary gas disc to black hole recoil and mass loss. / Corrales, Lia R.; Haiman, Zoltán; MacFadyen, Andrew.

    In: Monthly Notices of the Royal Astronomical Society, Vol. 404, No. 2, 05.2010, p. 947-962.

    Research output: Contribution to journalArticle

    Corrales, Lia R. ; Haiman, Zoltán ; MacFadyen, Andrew. / Hydrodynamical response of a circumbinary gas disc to black hole recoil and mass loss. In: Monthly Notices of the Royal Astronomical Society. 2010 ; Vol. 404, No. 2. pp. 947-962.
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