Resonance of Gaussian Electromagnetic Field to the High Frequency Gravitational Waves

Author(s)

Li, Jin ^{[1, 2]} ; Zhang, Lu ^{[1, 2]} ; Lin, Kai ^{[3, 4]} ; Wen, Hao ^{[1, 2]}

Affiliation

^[1] Chinese Acad Sci, Inst Theoret Phys, State Key Lab Theoret Phys, Beijing 100190 - Peoples R China

^[2] Chongqing Univ, Coll Phys, Chongqing 401331 - Peoples R China

^[3] Univ Fed Itajuba, Inst Fis & Quim, Itajuba, MG - Brazil

^[4] Univ Sao Paulo, Inst Fis, CP 66318, BR-05315970 Sao Paulo - Brazil

• Document type: Journal article
• Source: INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS; v. 55, n. 8, p. 3506-3514, AUG 2016.
• Web of Science Citations: 3

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. (AU)

• FAPESP's process: 12/08934-0 - Horava's gravity at Lifshitz fixed points and its applications to cosmology and astrophysics
• Grantee: Kai Lin
• Support Opportunities: Scholarships in Brazil - Post-Doctoral