Abstract
We consider a Gaussian Beam (GB) resonant system for high frequency gravitational waves (HFGWs) detection. At present, we find the optimal signal strength in theory through setting the magnetic component of GB in a standard gaussian form. Under the synchro-resonance condition, we study the signal strength (i.e., transverse perturbative photon fluxes) from the relic HFGWs (predicted by ordinary inflationary model) and the braneworld HFGWs (from braneworld scenarios). Both of them would generate potentially detectable transverse perturbative photon fluxes (PPFs). Furthermore we find optimal system parameters and the relationship between frequency and effective width of energy fluxes accumulation.
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Acknowledgments
This work is supported by FAPESP No. 2012/08934-0, CNPq, CAPES,National Natural Science Foundation of China No. 11205254, No. 11178018, No.11573022 and No.11375279, and the Fundamental Research Funds for the Central Universities 106112015CDJRC131216 and CDJRC10300003, and Chongqing Postdoctoral Science Foundation (No.Xm2015027), and the Open Project Program of State Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, China (No.Y5KF181CJ1).
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Li, J., Zhang, L., Lin, K. et al. Resonance of Gaussian Electromagnetic Field to the High Frequency Gravitational Waves. Int J Theor Phys 55, 3506–3514 (2016). https://doi.org/10.1007/s10773-016-2977-z
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DOI: https://doi.org/10.1007/s10773-016-2977-z