Negative dispersion medium at 1064 nm in an optomechanical resonator for enhancing the sensitivity bandwidth in a gravitational-wave detector
Minchuan Zhou, Selim M. Shahriar

TL;DR
This paper demonstrates a 1064nm negative dispersion medium using an optomechanical microresonator to enhance the bandwidth of gravitational-wave detectors, including a stabilization method for the system.
Contribution
It introduces a novel 1064nm optomechanical microresonator-based negative dispersion medium for gravitational-wave detectors, extending previous GEIT systems to operational wavelengths.
Findings
Achieved a sensitivity-bandwidth enhancement factor of ~15.
Implemented a feedback control to stabilize the optomechanical system.
Demonstrated negative dispersion at 1064nm in a microresonator.
Abstract
Recently, we had proposed an optically-pumped five-level Gain EIT (GEIT) system, which has a transparency dip superimposed on a gain profile and exhibits a negative dispersion suitable for the white light cavity (WLC) enhanced interferometric gravitational wave detector [Phys. Rev. D. 92, 082002 (2015)]. Using this system as the negative dispersion medium (NDM) in the WLC-SR (signal recycling) scheme, we get an enhancement in the quantum noise (QN) limited sensitivity-bandwidth product by a factor of ~18. We have also shown how to realize such a system in practice using Zeeman sublevels in Rb at 795nm [Opt. Commun. 402, 382-388 (2017)]. However, aLIGO operates at 1064nm and suitable transitions in Rb or other alkali atoms are not available at this wavelength. Therefore, it is necessary to consider a system that is consistent with the operating wavelength of aLIGO. Here, we…
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