TY - JOUR
T1 - Axion Dark Matter Search with Interferometrie Gravitational Wave Detectors
AU - Nagano, Koji
AU - Obata, Ippei
AU - Fujita, Tomohiro
AU - Michimura, Yuta
N1 - Funding Information:
In this work, KN, IO, YM and TF are supported by the JSPS KAKENHI Grant No. JP17J01176, JSPS KAKENHI Grant No. 19K14702, JSPS Grant-in-Aid for Scientific Research (B) No. 18H01224 and Grant-in-Aid for JSPS Research Fellow No. 17J09103, respectively.
Publisher Copyright:
© 2020 Published under licence by IOP Publishing Ltd.
PY - 2020/3/20
Y1 - 2020/3/20
N2 - 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 aγ, reaches g aγ ≃ 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 aγ ≃ 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.
AB - 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 aγ, reaches g aγ ≃ 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 aγ ≃ 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.
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U2 - 10.1088/1742-6596/1468/1/012027
DO - 10.1088/1742-6596/1468/1/012027
M3 - Conference article
AN - SCOPUS:85083103823
SN - 1742-6588
VL - 1468
JO - Journal of Physics: Conference Series
JF - Journal of Physics: Conference Series
IS - 1
M1 - 012027
T2 - 16th International Conference on Topics in Astroparticle and Underground Physics, TAUP 2019
Y2 - 9 September 2019 through 13 September 2019
ER -