dorsal/arxiv
View SchemaAdvanced configuration of gravitational-wave interferometer on the base of "sensitive mode" in "white-light cavity"
| Authors | G. G. Karapetyan |
|---|---|
| Categories | |
| ArXiv ID | physics/0211032 |
| URL | https://arxiv.org/abs/physics/0211032 |
| DOI | 10.1016/S0030-4018(03)01294-X |
Abstract
A novel conception of "sensitive mode" (SM) is proposed to apply in gravitational-wave advanced interferometer configuration. The SM is resonant oscillation of electromagnetic field in "white-light cavity", where the resonance line is broadened without decreasing cavity quality. The frequency of the SM is greatly susceptible to the change of cavity length, and the SM is established in a cavity with time constant smaller than a conventional mode. Due to these advantages the sensitivity and bandwidth of AIC can be increased.
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"abstract": "A novel conception of \"sensitive mode\" (SM) is proposed to apply in\ngravitational-wave advanced interferometer configuration. The SM is resonant\noscillation of electromagnetic field in \"white-light cavity\", where the\nresonance line is broadened without decreasing cavity quality. The frequency of\nthe SM is greatly susceptible to the change of cavity length, and the SM is\nestablished in a cavity with time constant smaller than a conventional mode.\nDue to these advantages the sensitivity and bandwidth of AIC can be increased.",
"arxiv_id": "physics/0211032",
"authors": [
"G. G. Karapetyan"
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"doi": "10.1016/S0030-4018(03)01294-X",
"title": "Advanced configuration of gravitational-wave interferometer on the base of \"sensitive mode\" in \"white-light cavity\"",
"url": "https://arxiv.org/abs/physics/0211032"
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