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Probing Majoron Dark Matter with Gravitational Wave Detectors
arXiv Physics
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이 매체는 공공·자유 라이선스로 본문을 직접 표시합니다.High Energy Physics - Phenomenology
[Submitted on 9 Apr 2026 (v1), last revised 18 Jun 2026 (this version, v2)]
Title:Probing Majoron Dark Matter with Gravitational Wave Detectors
View PDF HTML (experimental)Abstract:The Majoron is a hypothetical (pseudo) Nambu-Goldstone boson arising from the spontaneous breaking of a global lepton number symmetry, and is known as a candidate for dark matter in our Universe. In this paper, we investigate the possibility of probing the Majoron dark matter with a linear optical cavity used in the interferometric gravitational wave detectors. We consider a scenario in which the Majoron dark matter couples to photons through a QED anomaly, leading to an oscillatory photon birefringence induced by the coherent dark matter background. The anomaly coefficient is fixed by requiring the model to simultaneously reproduce the electroweak Higgs scale and a typical right-handed Majorana neutrino mass scale, and the resulting dark matter-photon coupling naturally falls within the sensitivity range of optical interferometers. By incorporating additional optics to extract the birefringence signal, we find that ground-based laser interferometers such as Advanced LIGO, KAGRA, as well as future detectors, can probe a region of the parameter space of Majoron dark matter.
Submission history
From: Ippei Obata [view email][v1] Thu, 9 Apr 2026 12:46:40 UTC (600 KB)
[v2] Thu, 18 Jun 2026 12:41:24 UTC (601 KB)
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