GEOPHYSICS, ASTRONOMY, AND ASTROPHYSICS |
Prev
|
|
|
Resonant behavior of stochastic oscillations of general relativistic disks driven by a memory-damped friction |
Wang Zhi-Yun (汪志云), Chen Pei-Jie (陈培杰), Zhang Liang-Ying (张良英) |
School of Physics and Electronic Engineering, Hubei University of Arts and Science, Xiangyang 441053, China |
|
|
Abstract By using a generalized Langevin equation to describe the vertical oscillations of a general relativistic disk subjected to a memory-damped friction and a stochastic force, we derive the power spectrum density (PSD) of accretion disk oscillating luminosity by the method of Laplace transform, and discuss the influence of the system parameters on the resonant behavior in PSD curves. The results show that as the damping strength α and memory time τ of the friction increase, the variation of PSD with spectrum frequency f from monotonous decreasing to occurring maximums, and the phenomenon of a general stochastic resonance (SR) with a single peak and multi-peaks can be found in PSD curves. The radial distance parameter n, the mass M, and spin parameter a* of the black hole determine the inherent frequency of vertical oscillations in the disk, and they have significant influences on the SR phenomena in a system of black hole binaries.
|
Received: 20 October 2014
Revised: 26 November 2014
Accepted manuscript online:
|
PACS:
|
98.62.Mw
|
(Infall, accretion, and accretion disks)
|
|
97.10.Sj
|
(Pulsations, oscillations, and stellar seismology)
|
|
97.60.Lf
|
(Black holes)
|
|
Fund: Project supported by the National Natural Science Foundation of China (Grant No. 11045004) and the Key Program of the Scientific Research Foundation of the Education Bureau of Hubei Province, China (Grant No. D20132603). |
Corresponding Authors:
Wang Zhi-Yun
E-mail: wzy425@126.com
|
About author: 98.62.Mw; 97.10.Sj; 97.60.Lf |
Cite this article:
Wang Zhi-Yun (汪志云), Chen Pei-Jie (陈培杰), Zhang Liang-Ying (张良英) Resonant behavior of stochastic oscillations of general relativistic disks driven by a memory-damped friction 2015 Chin. Phys. B 24 059801
|
[1] |
Shakura N I and Sunyaev R A 1973 Astron. Astrophys. 24 337
|
[2] |
Lynden-Bell D and Pringle J E 1974 Mon. Not. R. Astron. Soc. 168 603
|
[3] |
Remillard R A and Mcclintoc J E 2006 Astron. Astrophys. 44 49
|
[4] |
Mcclintoc J E and Remillard R A 2006 Black Hole Binaries (Cambridge: Cambridge Univ. Press) pp. 1-46
|
[5] |
Belloni T M, Sanna A and Méndez M 2012 Mon. Not. R. Astron. Soc. 426 1701
|
[6] |
Kato S 2001 Publ. Astron. Soc. Jpn. 53 1
|
[7] |
Abramowicz M A and Fragile P C 2013 Living Rev. Relativity 16 1
|
[8] |
Titarchuk L and Osherorich V 2000 Ap. J. 542 L111
|
[9] |
Blaes O M, Arras P and Fragile P C 2006 Mon. Not. R. Astron. Soc. 369 1235
|
[10] |
Kato S 1990 Publ. Astron. Soc. Jpn. 42 99
|
[11] |
Kato S 2008 Publ. Astron. Soc. Jpn. 60 111
|
[12] |
Ioannou P J and Kakouris A 2001 Ap. J. 550 931
|
[13] |
Das M K, Chaudhary A K and Tavakol R K 1996 Ap. J. 463 694
|
[14] |
Harko T and Mocanu G 2012 Mon. Not. R. Astron. Soc. 421 3102
|
[15] |
Harko T, Leung C S and Mocanu G 2014 Eur. Phys. J. C 74 2900
|
[16] |
Leung C S, Mocanu G and Harko T 2013 arXiv:1306.1078[astro-ph]
|
[17] |
Leung C S, Wei J Y, Harko T and Kovacs Z 2011 J. Astrophys. Astron. 32 189
|
[18] |
Wang Z Y, Chen P J, Wang D X and Zhang L Y 2013 J. Astrophys. Astron. 34 33
|
[19] |
Wang Z Y, Chen P J and Zhang L Y 2013 Chin. Phys. Lett. 30 099801
|
[20] |
Zhang L Y, Jin G X, Cao L and Wang Z Y 2012 Chin. Phys. B 12 120502
|
[21] |
Bao J D and Bai Z W 2005 Chin. Phys. Lett. 22 1845
|
[22] |
Bai Z W and Song Y L 2007 Acta Phys. Sin. 56 6220 (in Chinese)
|
No Suggested Reading articles found! |
|
|
Viewed |
|
|
|
Full text
|
|
|
|
|
Abstract
|
|
|
|
|
Cited |
|
|
|
|
Altmetric
|
blogs
Facebook pages
Wikipedia page
Google+ users
|
Online attention
Altmetric calculates a score based on the online attention an article receives. Each coloured thread in the circle represents a different type of online attention. The number in the centre is the Altmetric score. Social media and mainstream news media are the main sources that calculate the score. Reference managers such as Mendeley are also tracked but do not contribute to the score. Older articles often score higher because they have had more time to get noticed. To account for this, Altmetric has included the context data for other articles of a similar age.
View more on Altmetrics
|
|
|