Squeezed state generation for interferometric gravitational-wave detection
In this paper we present results demonstrating the development of a squeezed state at sideband frequencies as low as 100 Hz. The squeezed source was generated in a doubly resonant optical parametric oscillator (OPO) operated below threshold. The OPO resonance condition is achieved using the pump field, allowing the OPO to produce a squeezed vacuum state stably. We describe limitations to the experiment and discuss future work.
|Collections||ANU Research Publications|
|Source:||Classical and Quantum Gravity|
|01_McKenzie_Squeezed_state_generation_for_2006.pdf||146.91 kB||Adobe PDF||Request a copy|
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