|
|
High-frequency gravitational waves having large spectral densities and their electromagnetic response |
Li Fang-Yu (李芳昱), Wen Hao (文毫), Fang Zhen-Yun (方祯云) |
Department of Physics, Chongqing University, Chongqing 400044, China |
|
|
Abstract Various cosmology models, brane oscillation scenarios, interaction of interstellar plasma with intense electromagnetic radiation, and even high-energy physics experiments (e.g., Large Hadron Collider (LHC)) all predict high frequency gravitational waves (HFGWs, i.e., high-energy gravitons) in the microwave band and higher frequency region, and some of them have large energy densities. Electromagnetic (EM) detection to such HFGWs would be suitable due to very high frequencies and large energy densities of the HFGWs. We review several typical EM detection schemes, i.e., inverse Gertsenshtein effect (G-effect), coupling of the inverse G effect with a coherent EM wave, coupling of planar superconducting open cavity with a static magnetic field, cylindrical superconducting closed cavity, and the EM sychro-resonance system, and discuss related minimal detectable amplitudes and sensitivities. Furthermore, we give some new ideas and improvement ways enhancing the possibility of measuring the HFGWs. It is shown that there is still a large room for improvement for those schemes to approach and even reach up the requirement of detection of HFGWs expected by the cosmological models and high-energy astrophysical process.
|
Received: 09 April 2013
Revised: 20 May 2013
Accepted manuscript online:
|
PACS:
|
04.30.Nk
|
(Wave propagation and interactions)
|
|
04.25.Nx
|
(Post-Newtonian approximation; perturbation theory; related Approximations)
|
|
04.30.Db
|
(Wave generation and sources)
|
|
04.80.Nn
|
(Gravitational wave detectors and experiments)
|
|
Fund: Project supported by the National Natural Science Foundation of China (Grant Nos. 11075224 and 11375279) and the Foundation of China Academy of Engineering Physics (Grant Nos. 2008 T0401 and T0402). |
Corresponding Authors:
Li Fang-Yu
E-mail: fangyuli@cqu.edu.cn
|
Cite this article:
Li Fang-Yu (李芳昱), Wen Hao (文毫), Fang Zhen-Yun (方祯云) High-frequency gravitational waves having large spectral densities and their electromagnetic response 2013 Chin. Phys. B 22 120402
|
[1] |
Cuadrado G G 2009 AIP Conf. Proc. 1103 553
|
[2] |
Tong M L and Zhang Y 2009 Phys. Rev. D 80 084022
|
[3] |
Giovannini M 1999 Phys. Rev. D 60 123511
|
[4] |
Giovannini M 2009 Class. Quantum Grav. 26 045004
|
[5] |
Bisnovatyi-Kogun G S and Rudenko V R 2004 Class. Quantum Grav. 21 3347
|
[6] |
Cruise A M 2012 Class. Quantum Grav. 29 095003
|
[7] |
Press W H and Thorne K S 1972 Ann. Rev. Astron. Astrophys. 10 335
|
[8] |
Abbott B P, et al. 2009 Nature (London) 460 990
|
[9] |
Gasperini M and Veneziano G 2003 Phys. Rep. 373 1
|
[10] |
Veneziano G 2004 Sci. Am. 290 54
|
[11] |
Clarkson C and Seahra S S 2007 Class. Quantum Grav. 24 F33
|
[12] |
Servin M and Brodin G 2003 Phys. Rev. D 68 044017
|
[13] |
Sivaram C and Arun K 2011 arXiv: 0708.3343[astro-ph]
|
[14] |
Chen P 1994 Stanford Linear Accelerator Center Report (SLAC-PUB-6666) March 23, 1994, Rome, Italy, p. 379
|
[15] |
Wu X G and Fang Z Y 2008 Phys. Rev. D 78 094002
|
[16] |
Li F Y and Tang M X 2002 Int. J. Mod. Phys. D 11 1049
|
[17] |
Nikishov A I and Ritus V I 1990 Sov. Phys. JETP 71 643
|
[18] |
Chen P 1991 Mod. Phys. Lett. A 6 1069
|
[19] |
Gertsenshtein M E 1962 Sov. Phys. JETP 14 84
|
[20] |
Boccaletti D, De Sabbata V, Fortint P and Gualdi C 1970 Nuovo Cim. B 70 129
|
[21] |
De Logi W K and Mickelson A R 1977 Phys. Rev. D 16 2915
|
[22] |
Li F Y, Tang M X and Shi D P 2003 Phys. Rev. D 67 104008
|
[23] |
Li F Y, Yang N, Fang Z Y, Baker R M L Jr, Stephenson G and Wen H 2009 Phys. Rev. D 80 064013, arXiv: 0909.4118v2[gr-qc]
|
[24] |
Li J, Lin K, Li F Y and Zhong Y H 2011 Gen. Relativ. Gravit. 43 2209
|
[25] |
Li F Y and Baker R M L Jr 2007 Int. J. Mod. Phys. B 21 3274
|
[26] |
Li F Y, Chen Y and Wang P 2007 Chin. Phys. Lett. 24 3328
|
[27] |
Grishchuk L P and Sazin M V 1983 Sov. Phys. JETP 53 1128
|
[28] |
Grishchuk L P 2003 arXiv: gr-qc/0306013
|
[29] |
Bessonov E G 1998 arXiv: physics/9802037[physics.class-ph]
|
[30] |
Braginsky V B, Caves C M and Thorne K S 1977 Phys. Rev. D 15 2047
|
[31] |
Braginsky V B and Khalili F Y 1999 Phys. Lett. A 257 241
|
[32] |
Gerlach U H 1992 Phys. Rev. D 46 1239
|
[33] |
Woods R, Baker R M L Jr, Li F Y, Stephenson G V, Davis E W and Beckwith A W 2011 J. Mod. Phys. 2 498
|
[34] |
Yariv A 1989 Quantum Electronics, 3rd edn. (New York: Wiley)
|
[35] |
Li J, Li F Y and Zhong Y H 2009 Chin. Phys. B 18 922
|
[36] |
Stephenson G V 2009 AIP Conf. Proc. 1103 542
|
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
|
|
|