Probing neutrino magnetic moment at the Jinping neutrino experiment

Author:

Yue Baobiao,Liao Jiajun,Ling JiajieORCID

Abstract

Abstract Neutrino magnetic moment (νMM) is an important property of massive neutrinos. The recent anomalous excess at few keV electronic recoils observed by the XENON1T collaboration might indicate a ∼ 2.2 × 1011μB effective neutrino magnetic moment ($$ {\mu}_{\nu}^{\mathrm{eff}} $$ μ ν eff ) from solar neutrinos. Therefore, it is essential to carry out the νMM searches at a different experiment to confirm or exclude such a hypothesis. We study the feasibility of doing νMM measurement with 4 kton fiducial mass at Jinping neutrino experiment (Jinping) using electron recoil data from both natural and artificial neutrino sources. The sensitivity of $$ {\mu}_{\nu}^{\mathrm{eff}} $$ μ ν eff can reach < 1.2 × 1011μB at 90% C.L. with 10-year data taking of solar neutrinos. Besides the abundance of the intrinsic low energy background 14C and 85Kr in the liquid scintillator, we find the sensitivity to νMM is highly correlated with the systematic uncertainties of pp and 85Kr. Reducing systematic uncertainties (pp and 85Kr) and the intrinsic background (14C and 85Kr) can help to improve sensitivities below these levels and reach the region of astrophysical interest. With a 3 mega-Curie (MCi) artificial neutrino source 51Cr installed at Jinping neutrino detector for 55 days, it could give us a sensitivity to the electron neutrino magnetic moment ($$ {\mu}_{\nu_e} $$ μ ν e ) with < 1.1 × 1011μB at 90% C.L. . With the combination of those two measurements, the flavor structure of the neutrino magnetic moment can be also probed at Jinping.

Publisher

Springer Science and Business Media LLC

Subject

Nuclear and High Energy Physics

Reference53 articles.

1. L.B. Okun, M.B. Voloshin and M.I. Vysotsky, Electromagnetic Properties of Neutrino and Possible Semiannual Variation Cycle of the Solar Neutrino Flux, Sov. J. Nucl. Phys. 44 (1986) 440 [INSPIRE].

2. L.B. Okun, M.B. Voloshin and M.I. Vysotsky, Neutrino Electrodynamics and Possible Effects for Solar Neutrinos, Sov. Phys. JETP 64 (1986) 446 [INSPIRE].

3. C.-S. Lim and W.J. Marciano, Resonant Spin-Flavor Precession of Solar and Supernova Neutrinos, Phys. Rev. D 37 (1988) 1368 [INSPIRE].

4. E.K. Akhmedov, Resonant Amplification of Neutrino Spin Rotation in Matter and the Solar Neutrino Problem, Phys. Lett. B 213 (1988) 64 [INSPIRE].

5. H.O. Back et al., Study of the neutrino electromagnetic properties with prototype of Borexino detector, Phys. Lett. B 563 (2003) 35 [INSPIRE].

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