Development of a Displacement- and Frequency-Noise-Free Interferometer in a 3D Configuration for Gravitational Wave Detection

Keiko Kokeyama, Shuichi Sato, Atsushi Nishizawa, Seiji Kawamura, Yanbei Chen, and Akio Sugamoto
Phys. Rev. Lett. 103, 171101 – Published 22 October 2009

Abstract

The displacement- and frequency-noise-free interferometer (DFI) is a multiple laser interferometer array for gravitational-wave detection free from both the displacement noise of optics and laser frequency noise. So far, partial experimental demonstrations of the DFI have been done in 2D table top experiments. In this Letter, we report the complete demonstration of a 3D DFI. The DFI consists of four Mach-Zehnder interferometers with four mirrors and two beam splitters The attained maximum suppression of the displacement noise of both mirrors and beam splitters was 40 dB at about 50 MHz. The nonvanishing DFI response to a gravitational wave was successfully confirmed using multiple electro-optic modulators and computing methods.

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  • Received 5 June 2009

DOI:https://doi.org/10.1103/PhysRevLett.103.171101

©2009 American Physical Society

Authors & Affiliations

Keiko Kokeyama1,*, Shuichi Sato2, Atsushi Nishizawa3, Seiji Kawamura4, Yanbei Chen5, and Akio Sugamoto6

  • 1Graduate School of Humanities and Sciences, Ochanomizu University, 2-1-1, Otsuka, Bunkyo-ku, Tokyo 112-8610 Japan
  • 2Faculty of Engineering, Hosei University, 3-7-2, Kajino-cho, Koganei, Tokyo 184-8584 Japan
  • 3Graduate School of Human and Environmental Studies, Kyoto University, Kyoto 606-8501 Japan
  • 4TAMA project, National Astronomical Observatory of Japan, 2-21-1, Mitaka, Osawa, Tokyo 181-8588 Japan
  • 5Theoretical Astrophysics, California Institute of Technology, Pasadena, California 91125 USA
  • 6Ochanomizu University, 2-1-1, Otsuka, Bunkyo-ku, Tokyo 112-8610 Japan

  • *keiko.kokeyama@nao.ac.jp

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Vol. 103, Iss. 17 — 23 October 2009

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