Angular control of optical cavities in a radiation-pressure-dominated regime: the Enhanced LIGO case.
Angular control of optical cavities in a radiation-pressure-dominated regime: the Enhanced LIGO case.
复制标题
辐射压力主导状态下光学腔的角度控制:增强型 LIGO 案例。
DOI:
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发表时间:
2013
影响因子:
1.9
通讯作者:
N. Smith
中科院分区:
文献类型:
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作者:
K. Dooley;L. Barsotti;R. Adhikari;M. Evans;T. Fricke;P. Fritschel;V. Frolov;K. Kawabe;N. Smith
We describe the angular sensing and control (ASC) of 4 km detectors of the Laser Interferometer Gravitational-Wave Observatory (LIGO). Enhanced LIGO, the culmination of the first generation LIGO detectors, operated between 2009 and 2010 with about 40 kW of laser power in the arm cavities. In this regime, radiation-pressure effects are significant and induce instabilities in the angular opto-mechanical transfer functions. Here we present and motivate the ASC design in this extreme case and present the results of its implementation in Enhanced LIGO. Highlights of the ASC performance are successful control of opto-mechanical torsional modes, relative mirror motions of ≤ 1×10(-7) rad rms, and limited impact on in-band strain sensitivity.