Some properties of Kerr geometry with a repulsive cosmological constant

@inproceedings{43223,
   author = {Hledík, Stanislav and Petrásek, Martin},
   address = {Singapore},
   booktitle = {Eleventh Marcel Grossmann Meeting on General Relativity Berlin},
   keywords = {Stationary observers, Black hole, Kerr geometry, Cosmological constant, Kerr-de Sitter geometry},
   language = {eng},
   location = {Singapore},
   isbn = {978-981-283-426-3},
   publisher = {World Scientific},
   title = {Some properties of Kerr geometry with a repulsive cosmological constant},
   year = {2008}
}

TY  - JOUR
ID  - 43223
AU  - Hledík, Stanislav - Petrásek, Martin
PY  - 2008
TI  - Some properties of Kerr geometry with a repulsive cosmological constant
PB  - World Scientific
CY  - Singapore
SN  - 9789812834263
KW  - Stationary observers, Black hole, Kerr geometry, Cosmological constant, Kerr-de Sitter geometry
N2  - We summarize general properties of the Kerr-de Sitter geometry, i.e., Kerr geometry in the presence of a repulsive cosmological constant. An interesting difference between Kerr geometry and Kerr-de Sitter geometry has been found --- namely, the conditionof free fall (vanishing 4-acceleration) is satisfied for stationary observers located on the axis of symmetry above the horizon.
ER  - 

HLEDÍK, Stanislav a Martin PETRÁSEK. Some properties of Kerr geometry with a repulsive cosmological constant. In \textit{Eleventh Marcel Grossmann Meeting on General Relativity Berlin}. Singapore: World Scientific, 2008, 3 s. ISBN~978-981-283-426-3.