Epicyclic oscillations of fluid bodies:: II.: Strong gravity

被引:49
作者
Abramowicz, MA [1 ]
Blaes, OM
Horák, J
Kluzniak, W
Rebusco, P
机构
[1] Univ Gothenburg, Dept Phys, S-41296 Gothenburg, Sweden
[2] Copernicus Astron Ctr, PL-00716 Warsaw, Poland
[3] NORDITA, DK-2100 Copenhagen, Denmark
[4] Univ Calif Santa Barbara, Kavli Inst Theoret Phys, Santa Barbara, CA 93106 USA
[5] Univ Paris 06, CNRS, UMR 7095, Inst Astrophys, F-75014 Paris, France
[6] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA
[7] Acad Sci Czech Republ, Inst Astron, CZ-14131 Prague, Czech Republic
[8] Zielona Gora Univ, Inst Astron, PL-65265 Zielona Gora, Poland
[9] Max Planck Inst Astrophys, D-85741 Garching, Germany
关键词
D O I
10.1088/0264-9381/23/5/014
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Fluids in external gravity may oscillate with frequencies characteristic of the epicyclic motions of test particles. We explicitly demonstrate that global oscillations of a slender, perfect fluid torus around a Kerr black hole admit incompressible vertical and radial epicyclic modes. Our results may be directly relevant to one of the most puzzling astrophysical phenomena-high (hundreds of hertz) frequency quasiperiodic oscillations (QPOs) detected in x-ray fluxes from several black hole sources. Such QPOs are pairs of stable frequencies in the 3/2 ratio. It seems that they originate a few gravitational radii away from the black hole and thus their observations have the potential to become an accurate probe of super-strong gravity.
引用
收藏
页码:1689 / 1696
页数:8
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