Integrability of Geodesics in Near-Horizon Extremal Vanishing Horizon Myers–Perry Black Holes
- Authors: Demirchyan H.1, Nersessian A.2,3,4, Sadeghian S.5, Sheikh-Jabbari M.M.5
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Affiliations:
- Byurakan Astrophysical Observatory
- Yerevan Physics Institute
- Joint Institute for Nuclear Research
- Yerevan State University
- Institute for Research in Fundamental Sciences (IPM)
- Issue: Vol 81, No 6 (2018)
- Pages: 907-911
- Section: Elementary Particles and Fields
- URL: https://journal-vniispk.ru/1063-7788/article/view/196133
- DOI: https://doi.org/10.1134/S106377881806011X
- ID: 196133
Cite item
Abstract
We study geodesics on the near horizon geometry of odd-dimensional Myers–Perry black hole in the extremal vanishing horizon (EVH) limit. Knowing the fact that geodesics equations on Myers–Perry black hole are integrable in ellipsoidal coordinates, we take the near horizon limit in this coordinate system and obtain the near horizon EVH geometry and its Killing tensors. We explicitly show that geodesics equations are integrable on the near horizon EVH geometry ofMyers–Perry and compute the constants of motion. The resultant Killing tensors of this constants of motion matches with the Killing tensors given by taking the near-horizon limit.
About the authors
H. Demirchyan
Byurakan Astrophysical Observatory
Author for correspondence.
Email: demhov@bao.sci.am
Armenia, Byurakan
A. Nersessian
Yerevan Physics Institute; Joint Institute for Nuclear Research; Yerevan State University
Email: demhov@bao.sci.am
Armenia, Yerevan, 0036; Dubna; Yerevan, 0025
S. Sadeghian
Institute for Research in Fundamental Sciences (IPM)
Email: demhov@bao.sci.am
Iran, Islamic Republic of, Tehran
M. M. Sheikh-Jabbari
Institute for Research in Fundamental Sciences (IPM)
Email: demhov@bao.sci.am
Iran, Islamic Republic of, Tehran
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