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    Marginally stable thick discs orbiting the Kerr-de Sitter black holes: the mass estimates

    Zdeněk Stuchlík · Duben 01, 2007 · Fyzika · 0 comments
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    Publication date: Apr 2007

    Abstract:
    Properties of equipotential surfaces in test perfect fluid tori with
    uniform distribution of the specific angular momentum orbiting KdS black
    holes will be summarized. The last closed surface crosses itself in the
    cusp(s) enabling outflow(s) of matter from the torus. The repulsive
    (positive) cosmological constant is responsible for the existence of the
    outer cusp (with a stabilizing effect on the tori because of the
    excretion) and strong collimation of open equipotential surfaces along
    the rotational axis. We shall present the mass estimates for tori with
    an adiabatic equation of state enabling to put limits on their central
    mass density, for which the approximation of test fluid is adequate.

    Authors:
    Slaný, Petr; Stuchlík, Zdeněk;

    http://adsabs.harvard.edu/abs/2007IAUS..238..449S

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