Sub-hertz optomechanically induced transparency with a kilogram-scale mechanical oscillator

Sub-hertz optomechanically induced transparency with a kilogram-scale mechanical oscillator
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DOI:
10.1103/physreva.100.013853
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发表时间:
2018-12
期刊:
影响因子:
2.9
通讯作者:
T. Bodiya;V. Sudhir;C. Wipf;N. Smith;A. Buikema;A. Kontos;Hang Yu;N. Mavalvala
T. Bodiya;V. Sudhir;C. Wipf;N. Smith;A. Buikema;A. Kontos;Hang Yu;N. Mavalvala
中科院分区:
物理与天体物理2区
文献类型:
--
作者:
T. Bodiya;V. Sudhir;C. Wipf;N. Smith;A. Buikema;A. Kontos;Hang Yu;N. Mavalvala

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Optical interferometers with suspended mirrors are the archetype of all current audio-frequency gravitational-wave detectors. The radiation pressure interaction between the motion of the mirrors and the circulating optical field in such interferometers represents a pristine form of light-matter coupling, largely due to 30 years of effort in developing high-quality optical materials with low mechanical dissipation. However, in all current suspended interferometers, the radiation pressure interaction is too weak to be useful as a resource, and too strong to be neglected. Here, we demonstrate a meter-long interferometer with suspended mirrors, of effective mass $125\phantom{\rule{0.28em}{0ex}}\mathrm{g}$, where the radiation pressure interaction is enhanced by strong optical pumping to realize a cooperativity of 50. In conjunction with modest resolved-sideband operation, this regime is efficiently probed via optomechanically induced transparency of a weak on-resonant probe. The low resonant frequency and high-Q of the mechanical oscillator allows us to demonstrate transparency windows barely 100 mHz wide at room temperature. Together with a near-unity ($\ensuremath{\approx}99.9%$) out-coupling efficiency, our system saturates the theoretical delay-bandwidth product, rendering it an optical buffer capable of seconds-long storage times.