J
2009
Profiles of emission lines generated by rings orbiting braneworld Kerr black holes
SCHEE, Jan and Zdeněk STUCHLÍK
Basic information
Original name
Profiles of emission lines generated by rings orbiting braneworld Kerr black holes
Edition
General Relativity and Gravitation, US - Spojené státy americké, 2009, 1572-9532
Other information
Type of outcome
Článek v odborném periodiku
Field of Study
10308 Astronomy
Confidentiality degree
není předmětem státního či obchodního tajemství
Organization unit
Faculty of Philosophy and Science in Opava
Keywords in English
black hole, emmision line, brany model
Tags
International impact, Reviewed
Links
MSM4781305903, plan (intention).
V originále
In the framework of the braneworld models, rotating black holes can be described by the Kerr metric with a tidal charge representing the influence of the non-local gravitational (tidal) effects of the bulk space Weyl tensor onto the black hole spacetime.We study the influence of the tidal charge onto profiled spectral lines generated by radiating tori orbiting in vicinity of a rotating black hole. We show that with lowering the negative tidal charge of the black hole, the profiled line becomes to be flatter and wider keeping their standard character with flux stronger at the blue edge of the profiled line. The extension of the line grows with radius falling and inclination angle growing.
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