Holonomy invariance, orbital resonances and kilohertz QPOs

被引:14
作者
Abramowicz, MA [1 ]
Almergren, GJE
Kluzniak, W
Thampan, AV
Wallinder, F
机构
[1] Chalmers Univ, Dept Astron & Astrophys, S-41296 Gothenburg, Sweden
[2] SISSA, Int Sch Adv Studies, I-34014 Trieste, Italy
[3] Zielona Gora Univ, Inst Astron, PL-65365 Zielona Gora, Poland
[4] Univ Orebro, Dept Nat Sci, S-70182 Orebro, Sweden
关键词
D O I
10.1088/0264-9381/19/8/103
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Quantized orbital structures are typical for many aspects of classical gravity (Newton's as well as Einstein's). The astronomical phenomenon of orbital resonances is a well-known example. Recently, Rothman et al (2001 Class. Quantum Grav. 18 1217-33) discussed quantized orbital structures in the novel context of a holonomy invariance of parallel transport in Schwarzschild geometry. We present here yet another example of quantization of orbits, one that is closely related to orbital resonances and closely analogous to holonomy invariance. This strong-gravity effect may have been already directly observed as the puzzling kilohertz quasi-periodic oscillations (QPOs) in the x-ray emission from a few accreting galactic black holes and several neutron stars.
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页码:L57 / L61
页数:5
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