Torsion-bar antenna in the proper reference frame with rotation

Kouji Nakamura and Masaki Ando
Phys. Rev. D 90, 064008 – Published 4 September 2014

Abstract

The resultant response of the rotating torsion-bar antenna for gravitational waves discussed in M. Ando et al. [Phys. Rev. Lett. 105, 161101 (2010)] is reinvestigated from a general-relativistic point of view. To do this, the equation of motion of a free-falling particle in the proper reference frame of a rotating observer is used. As a result, the resultant response derived in the above paper is also valid even when ωgΩ, where ωg and Ω are the angular frequencies of gravitational waves and the rotation of the antenna, respectively.

  • Received 15 May 2014

DOI:https://doi.org/10.1103/PhysRevD.90.064008

© 2014 American Physical Society

Authors & Affiliations

Kouji Nakamura1,* and Masaki Ando1,2

  • 1TAMA Project Office, Optical and Infrared Astronomy Division, National Astronomical Observatory, Osawa 2-21-1, Mitaka, Tokyo 181-8588, Japan
  • 2Department of Physics, The University of Tokyo, Hongo 7-3-1, Tokyo 113-0033, Japan

  • *kouji.nakamura@nao.ac.jp

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Issue

Vol. 90, Iss. 6 — 15 September 2014

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