| GENERAL |
|
|
|
|
Electromagnetic Resonance of Astigmatic Gaussian Beam to the High Frequency Gravitational Waves |
| Yuan-Hong Zhong1**, Jin Li2, Yao Zhou1, Qi-Lun Lei1 |
1College of Communication Engineering, Chongqing University, Chongqing 400044
2College of Physics, Chongqing University, Chongqing 401331
|
|
| Cite this article: |
|
Yuan-Hong Zhong, Jin Li, Yao Zhou et al 2016 Chin. Phys. Lett. 33 100402 |
|
|
|
|
Abstract The high frequency gravitational waves (around $10^{8}$–$10^{12}$ Hz) could interact with a specially designed electromagnetic resonance system. It is found that the power of transverse perturbative photon flux (PPF) of an electromagnetic resonance system can be improved significantly by virtue of an astigmatic Gaussian beam. Correspondingly the signal-to-noise ratio (SNR) would also be improved. When the eccentric ratio of waist satisfying $w_{0x}:w_{0y}>1$, the peak value of signal photon flux could be raised by 2–4 times with typical systematic parameters, while the background photon flux would be depressed. Therefore, the ratio of transverse PPF to background photon flux (i.e., SNR) can be further improved 3–8 times with dimensionless amplitude of relic gravitational wave $h_{\rm t}=10^{-36}$.
|
|
|
Received: 14 July 2016
Published: 27 October 2016
|
|
| 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)
|
|
|
| Fund: Supported by the National Natural Science Foundation of China under Grant Nos 11205254 and 61501069, and the Fundamental Research Funds for the Central Universities under Grant No 106112016CDJXY300002. |
|
|
|
|
Viewed |
|
|
|
Full text
|
|
|
|
|
Abstract
|
|
|
|
|
