KUČÁKOVÁ, Hana, Daniela PUGLIESE, Jan SCHEE a Zdeněk STUCHLÍK. Perfect fluid tori orbiting Kehagias-Sfetsos naked singularities. The European Physical Journal C. US - Spojené státy americké, 2015, roč. 75, č. 9, s. "451-1"-"451-31", 31 s. ISSN 1434-6044. Dostupné z: https://dx.doi.org/10.1140/epjc/s10052-015-3663-7. |
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@article{46123, author = {Kučáková, Hana and Pugliese, Daniela and Schee, Jan and Stuchlík, Zdeněk}, article_location = {US - Spojené státy americké}, article_number = {9}, doi = {http://dx.doi.org/10.1140/epjc/s10052-015-3663-7}, keywords = {naked singularity; accretion; perfect fluid tori}, language = {eng}, issn = {1434-6044}, journal = {The European Physical Journal C}, title = {Perfect fluid tori orbiting Kehagias-Sfetsos naked singularities}, url = {https://link.springer.com/article/10.1140/epjc/s10052-015-3663-7}, volume = {75}, year = {2015} }
TY - JOUR ID - 46123 AU - Kučáková, Hana - Pugliese, Daniela - Schee, Jan - Stuchlík, Zdeněk PY - 2015 TI - Perfect fluid tori orbiting Kehagias-Sfetsos naked singularities JF - The European Physical Journal C VL - 75 IS - 9 SP - "451-1"-"451-31" EP - "451-1"-"451-31" SN - 14346044 KW - naked singularity KW - accretion KW - perfect fluid tori UR - https://link.springer.com/article/10.1140/epjc/s10052-015-3663-7 N2 - We construct perfect fluid tori in the field of the Kehagias-Sfetsos (K-S) naked singularities. These are spherically symmetric vacuum solutions of the modified Horava quantum gravity, characterized by a dimensionless parameter omega M^2, combining the gravitational mass parameter M of the spacetime with the Horava parameter., reflecting the role of the quantum corrections. In dependence on the value of omega M^2, the K-S naked singularities demonstrate a variety of qualitatively different behavior of their circular geodesics that is fully reflected in the properties of the toroidal structures, demonstrating clear distinction to the properties of the torii in the Schwarzschild spacetimes. In all of the K-S naked singularity spacetimes the tori are located above an "antigravity" sphere where matter can stay in a stable equilibrium position, which is relevant for the stability of the orbiting fluid toroidal accretion structures. The signature of the K-S naked singularity is given by the ER -
KUČÁKOVÁ, Hana, Daniela PUGLIESE, Jan SCHEE a Zdeněk STUCHLÍK. Perfect fluid tori orbiting Kehagias-Sfetsos naked singularities. \textit{The European Physical Journal C}. US - Spojené státy americké, 2015, roč.~75, č.~9, s.~''451-1''-''451-31'', 31 s. ISSN~1434-6044. Dostupné z: https://dx.doi.org/10.1140/epjc/s10052-015-3663-7.
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