High-frequency gravitational waves having large spectral densities and their electromagnetic response

doi:10.1088/1674-1056/22/12/120402

中国物理B ›› 2013, Vol. 22 ›› Issue (12): 120402-120402.doi: 10.1088/1674-1056/22/12/120402

High-frequency gravitational waves having large spectral densities and their electromagnetic response

李芳昱, 文毫, 方祯云

Department of Physics, Chongqing University, Chongqing 400044, China

收稿日期:2013-04-09 修回日期:2013-05-20 出版日期:2013-10-25 发布日期:2013-10-25
基金资助:
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).

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

Received:2013-04-09 Revised:2013-05-20 Online:2013-10-25 Published:2013-10-25
Contact: Li Fang-Yu E-mail:fangyuli@cqu.edu.cn
Supported by:
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).

摘要/Abstract

摘要： 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.

关键词: high-frequency gravitational waves, electromagnetic response of high-frequency gravitational waves, superconducting microwave cavities, synchro-resonance system

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.

Key words: high-frequency gravitational waves, electromagnetic response of high-frequency gravitational waves, superconducting microwave cavities, synchro-resonance system

中图分类号: (Wave propagation and interactions)

04.30.Nk

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)

李芳昱, 文毫, 方祯云. High-frequency gravitational waves having large spectral densities and their electromagnetic response[J]. 中国物理B, 2013, 22(12): 120402-120402.

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[J]. Chin. Phys. B, 2013, 22(12): 120402-120402.

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High-frequency gravitational waves having large spectral densities and their electromagnetic response

High-frequency gravitational waves having large spectral densities and their electromagnetic response

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