Published July 29, 2022 | Version v1

Optical design of a mode cleaner for a small-scale suspended interferometer for quantum noise reduction in gravitational wave detectors

  • 1. Dipartimento di Fisica, Università di Roma "La Sapienza", P.vle Aldo Moro 5, 00185, Roma, Italy; INFN, Sezione di Roma, P.le Aldo Moro 2, 00185, Roma, Italy
  • 2. Dipartimento di Fisica, Università di Napoli "Federico II" and INFN Sezione di Napoli, Complesso Universitario di Monte Sant'Angelo, V. Cinthia 21, 80126, Napoli, Italy
  • 3. KASI(Korea Astronomy and Space Science Institute), 776 Daedeok-daero, Yuseong-gu, Daejeon 34055, Republic of Korea

Description

A mode cleaner optical cavity is a resonator that can be tuned to transmit a desired transverse mode present in the incoming beam, suppressing all the others. We present the optical design of a suited input mode cleaner for a small-scale Michelson interferometer, called SIPS (Suspended Interferometer for Ponderomotive Squeezing). The physical goal is to feed SIPS with a beam with a Gaussian profile, which also ensures a highly focused beam along the propagation axis. The SIPS mode cleaner has been designed to have a maximum circulating power of 130W, and to deliver a transmitted power of at least 2.5W in input of SIPS interferometer. It guarantees a suppression factor of at least 20 dB for every tested higher order mode. This work is framed within the implementation of a table-top optical experiment to test the broadband Quantum Noise reduction in the SIPS sensitivity curve, via frequency-dependent squeezing achieved by employing Einstein-Podolsky-Rosen quantum entangled states of light.

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