| Full text | |
| Author(s): |
Total Authors: 2
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| Affiliation: | [1] Chongqing Univ, Dept Phys, Chongqing 401331 - Peoples R China
Total Affiliations: 1
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| Document type: | Journal article |
| Source: | GRAVITATION & COSMOLOGY; v. 24, n. 1, p. 22-27, JAN 2018. |
| Web of Science Citations: | 0 |
| Abstract | |
Transverse perturbative photon fluxes (PPFs) generated by an electromagnetic (EM) response system for high-frequency gravitational waves (HFGWs) detection, is a special physical effect related to some properties of HFGWs. Meanwhile, it is also influenced by the background static magnetic field. In this paper, based on the relationship between PPFs and the distribution of a Gaussian Beam with a homogeneous background static magnetic field, we study the distribution of PPFs and the width of positive signal photon fluxes with an inhomogeneous background static magnetic field. Under this condition, the strength of PPFs is enhanced significantly. Furthermore, by adjusting some parameters and an embedded non-coaxial coil in the background magnetic coil, the width of positive-signal photon fluxes would be enlarged greatly. (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 |