@article{44083,
   author = {Slaný, Petr and Stuchlík, Zdeněk},
   article_location = {US - Spojené státy americké},
   article_number = {17},
   doi = {http://dx.doi.org/10.1088/0264-9381/22/17/019},
   keywords = {Relativistic, thick discs, Kerr de Sitter backgrounds, perfect fluid},
   language = {eng},
   issn = {0264-9381},
   journal = {Classical and Quantum Gravity},
   title = {Relativistic thick discs in the Kerr de Sitter backgrounds},
   volume = {22},
   year = {2005}
}

TY  - JOUR
ID  - 44083
AU  - Slaný, Petr - Stuchlík, Zdeněk
PY  - 2005
TI  - Relativistic thick discs in the Kerr de Sitter backgrounds
JF  - Classical and Quantum Gravity
VL  - 22
IS  - 17
SP  - 3623-3651
EP  - 3623-3651
SN  - 02649381
KW  - Relativistic, thick discs, Kerr de Sitter backgrounds, perfect fluid
N2  - Perfect fluid tori with a uniform distribution of the specific angular momentum, l(r,theta) = const, orbiting the Kerr - de Sitter black holes or naked singularities are studied. It is well known that the structure of equipotential surfaces of such marginally stable tori reflects the basic properties of any tori with a general distribution of the specific angular momentum. Closed equipotential surfaces corresponding to stationary thick discs are allowed only in the spacetimes admitting stable circular geodesics. The last closed surface crosses itself in the cusp(s) enabling the outflow of matter from the torus due to the violation of hydrostatic equilibrium.
ER  - 

SLANÝ, Petr and Zdeněk STUCHLÍK. Relativistic thick discs in the Kerr de Sitter backgrounds. \textit{Classical and Quantum Gravity}. US - Spojené státy americké, 2005, vol.~22, No~17, p.~3623-3651, 28 pp. ISSN~0264-9381. Available from: https://dx.doi.org/10.1088/0264-9381/22/17/019.