Observation and characterization of an optical spring
被引:161
作者:
Sheard, BS
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机构:
Australian Natl Univ, Fac Sci, Dept Phys, Ctr Gravitat Phys, Acton, ACT 0200, AustraliaAustralian Natl Univ, Fac Sci, Dept Phys, Ctr Gravitat Phys, Acton, ACT 0200, Australia
Sheard, BS
[1
]
Gray, MB
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机构:Australian Natl Univ, Fac Sci, Dept Phys, Ctr Gravitat Phys, Acton, ACT 0200, Australia
Gray, MB
Mow-Lowry, CM
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机构:Australian Natl Univ, Fac Sci, Dept Phys, Ctr Gravitat Phys, Acton, ACT 0200, Australia
Mow-Lowry, CM
McClelland, DE
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机构:Australian Natl Univ, Fac Sci, Dept Phys, Ctr Gravitat Phys, Acton, ACT 0200, Australia
McClelland, DE
Whitcomb, SE
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机构:Australian Natl Univ, Fac Sci, Dept Phys, Ctr Gravitat Phys, Acton, ACT 0200, Australia
Whitcomb, SE
机构:
[1] Australian Natl Univ, Fac Sci, Dept Phys, Ctr Gravitat Phys, Acton, ACT 0200, Australia
[2] CALTECH, LIGO Lab, Pasadena, CA 91125 USA
来源:
PHYSICAL REVIEW A
|
2004年
/
69卷
/
05期
关键词:
D O I:
10.1103/PhysRevA.69.051801
中图分类号:
O43 [光学];
学科分类号:
070207 ;
0803 ;
摘要:
Recent theoretical developments have highlighted the potential importance of "optical springs" in interferometers for gravitational wave detection as a means for beating the standard quantum limit. We have observed an optical spring effect experimentally in a detuned Fabry-Perot resonator in which one mirror is mounted on a flexure so that it has a significant response to radiation pressure. The main effect of the optical spring, an observed shift in the mechanical resonance frequency of the moveable mirror, agrees well with a simple model.