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Electrogravitational Resonance of a Gaussian Beam to a High-Frequency Relic Gravitational Wave |
| LI Fang-Yu1;TANG Meng-Xi2 |
| 1Department of Physics, Chongqing University, Chongqing 400044
2Department of Physics, Zhongshan University, Guangzhou 510275
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| Cite this article: |
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LI Fang-Yu, TANG Meng-Xi 2001 Chin. Phys. Lett. 18 1546-1549 |
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Abstract We consider the resonant response of a Gaussian beam passing through a static magnetic field to a high-frequency relic gravitational wave (GW). It is found that under the synchroresonance condition, the first-order perturbative electromagnetic energy fluxes will contain a “left circularly wave” and a “right circularly wave”around the symmetrical axis of the Gaussian beam, but the perturbative effects produced by the + and x polarization of the GW have different physical behaviour. For the high-frequency relic GW with vg = 1010Hz, h = 10-30, recently expected by the quintessential inflationary models, the corresponding perturbative photon flux passing through the region 10-2m2 would be expected to be 104s-1, This is the largest perturbative photon flux we recently analysed and estimated using the typical laboratory parameters.
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| Keywords:
04.80.Nn
04.30.Nk
04.30.Db
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Published: 01 December 2001
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| PACS: |
04.80.Nn
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(Gravitational wave detectors and experiments)
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04.30.Nk
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(Wave propagation and interactions)
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04.30.Db
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(Wave generation and sources)
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