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    Observational phenomena related to primordial Kerr superspinars

    Zdeněk Stuchlík · Březen 01, 2012 · Fyzika · 0 comments
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    Publication date: Mar 2012

    Abstract:
    String theory indicates the existence of primordial Kerr superspinars,
    extremely compact objects with exterior described by the Kerr naked-
    singularity geometry. The primordial superspinars have to be converted
    to a black hole due to accretion, but they could survive to the era of
    high-redshift quasars. We discuss observational phenomena caused by the
    primordial Kerr superspinars in this era, considering the properties of
    corotating Keplerian accretion discs orbiting such superspinars and the
    optical phenomena modified by their presence. The potential well around
    a near-extreme superspinar with spin a very close to the extreme black
    hole value a = 1 is very deep so that the efficiency of the accretion
    process reaches 157.7%, influencing thus significantly the spectral
    continuum of corotating Keplerian discs and giving a signature of near-
    extreme superspinars. Such superspinars can also serve as an efficient
    accelerator for extremely high-energy collisions. Phenomena enabling a
    clear distinction of primordial Kerr superspinars and black holes are
    related to the disc oscillations with the radial and vertical epicyclic
    frequencies and the most profound could be differences implied by the
    profiled spectral lines generated in the innermost parts of the
    corotating Keplerian discs.

    Authors:
    Stuchlík, Zdeněk; Schee, Jan;

    https://ui.adsabs.harvard.edu/abs/2012CQGra..29f5002S

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