Resonance of Gaussian Electromagnetic Field to the High Frequency Gravitational Waves期刊界 All Journals 搜尽天下杂志传播学术成果专业期刊搜索期刊信息化学术搜索

Resonance of Gaussian Electromagnetic Field to the High Frequency Gravitational Waves

Authors:	Jin?Li author-information" > author-information__contact u-icon-before" > mailto:cqstarv@hotmail.com" title=" cqstarv@hotmail.com" itemprop=" email" data-track=" click" data-track-action=" Email author" data-track-label=" " >Email author,Lu?Zhang,Kai?Lin,Hao?Wen

Affiliation:	1.College of Physics,Chongqing University,Chongqing,China;2.State Key Laboratory of Theoretical Physics, Institute of Theoretical Physics,Chinese Academy of Sciences,Beijing,China;3.Instituto de Física e Química,Universidade Federal de Itajubá,Itajubá,Brasil;4.Instituto de Física,Universidade de S?o Paulo,S?o Paulo,Brazil

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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