The Use of Cryogenic Techniques to Achieve High Sensitivity in Gravitational Wave Detectors
Cryogenic detectors for gravitational wave astronomy promise greatly improved sensitivity over room temperature detectors. The 3 mK detector which we have under construction should give an improvement of 10 6 over existing detectors. The cryogenic antennae are described and the calculated low temper...
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| Veröffentlicht in: | Symposium - International Astronomical Union 1974, Vol.64, p.40-51 |
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| container_title | Symposium - International Astronomical Union |
| container_volume | 64 |
| creator | Boughn, S. P. Fairbank, W. M. McASHAN, M. S. Paik, H. J. Taber, R. C. Bernat, T. P. Blair, D. G. Hamilton, W. O. |
| description | Cryogenic detectors for gravitational wave astronomy promise greatly improved sensitivity over room temperature detectors. The 3 mK detector which we have under construction should give an improvement of 10
6
over existing detectors. The cryogenic antennae are described and the calculated low temperature performance is detailed. New superconducting instrumentation is described. |
| doi_str_mv | 10.1017/S0074180900235985 |
| format | Article |
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6
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| identifier | ISSN: 0074-1809 |
| ispartof | Symposium - International Astronomical Union, 1974, Vol.64, p.40-51 |
| issn | 0074-1809 |
| language | eng |
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| source | Alma/SFX Local Collection |
| title | The Use of Cryogenic Techniques to Achieve High Sensitivity in Gravitational Wave Detectors |
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