Axion Dark Matter Search with Interferometrie Gravitational Wave Detectors

Koji Nagano, Ippei Obata, Tomohiro Fujita, Yuta Michimura

Research output: Contribution to journalConference articlepeer-review

Abstract

Axion dark matter differentiates the phase velocities of the circular-polarized photons. In [Phys. Rev. Lett. 123, 111301 (2019)], we have proposed a scheme to measure the phase difference by using a linear optical cavity. If the scheme is applied to the Fabry-Perot arm of Advanced LIGO-like (Cosmic-Explorer-like) gravitational wave detector, the potential sensitivity to the axion-photon coupling constant, g , reaches g ≃ 8 10-13 GeV-1 (4 10-14 GeV-1) at the axion mass m ≃ 3 10-13 eV (2 10-15 eV) and remains at around this sensitivity for 3 orders of magnitude in mass. Furthermore, its sensitivity has a sharp peak reaching g ≃ 10-14 GeV-1 (8 10-17 GeV-1) at m = 1.563 10-10 eV (1.563 10-11 eV). This sensitivity can be achieved without loosing any sensitivity to gravitational waves.

Original languageEnglish
Article number012027
JournalJournal of Physics: Conference Series
Volume1468
Issue number1
DOIs
Publication statusPublished - 2020 Mar 20
Externally publishedYes
Event16th International Conference on Topics in Astroparticle and Underground Physics, TAUP 2019 - Toyama, Japan
Duration: 2019 Sep 92019 Sep 13

ASJC Scopus subject areas

  • Physics and Astronomy(all)

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