Search engine for discovering works of Art, research articles, and books related to Art and Culture
ShareThis
Javascript must be enabled to continue!

Probing neutrino magnetic moment at the Jinping neutrino experiment

View through CrossRef
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 × 10−11μB 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 × 10−11μB 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 × 10−11μB 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.
Title: Probing neutrino magnetic moment at the Jinping neutrino experiment
Description:
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 × 10−11μB 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 × 10−11μB 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 × 10−11μB 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.

Related Results

Effectiveness and Timing of Congenital Nasolacrimal Duct Obstruction Probing: a Systematic Review
Effectiveness and Timing of Congenital Nasolacrimal Duct Obstruction Probing: a Systematic Review
Abstract Introduction & Objectives : Most congenital nasolacrimal duct obstruction (NLDO) cases could resolve spontaneously or only require minimal conservative treatment...
Magnetic cloak made of NdFeB permanent magnetic material
Magnetic cloak made of NdFeB permanent magnetic material
In the past few years, the concept of an electromagnetic invisibility cloak has received much attention. Based on the pioneering theoretical work, invisibility cloaks have been gre...
Investigating Sterile Neutrino Flux in the Solar Neutrino Data
Investigating Sterile Neutrino Flux in the Solar Neutrino Data
There are compelling evidences for the existence of a fourth degree of freedom of neutrinos, i.e., sterile neutrino. In the recent studies the role of sterile component of neutrino...
Neutrino Oscillation Effects on the Luminosity of Neutrino-dominated Accretion Flows around Black Holes
Neutrino Oscillation Effects on the Luminosity of Neutrino-dominated Accretion Flows around Black Holes
Abstract A stellar-mass black hole surrounded by the neutrino-dominated accretion flow (NDAF) has been proposed as the central engine of gamma-ray bursts. In this wo...
Constraints on Populations of Neutrino Sources from Searches in the Directions of IceCube Neutrino Alerts
Constraints on Populations of Neutrino Sources from Searches in the Directions of IceCube Neutrino Alerts
Abstract Beginning in 2016, the IceCube Neutrino Observatory has sent out alerts in real time containing the information of high-energy (E ≳ 100 TeV) neutrino candid...
Analysis of magnetohydrodynamic drag character for hypersonic vehicles
Analysis of magnetohydrodynamic drag character for hypersonic vehicles
In hypersonic flight, a very high temperature area can form ahead of the nose of aerocraft due to the shock aerodynamic heating, which leads to air weakly ionized. Many researchers...
Yifang Wang: high energy physics in China
Yifang Wang: high energy physics in China
Abstract On 8 March 2012, Yifang Wang, co-spokesperson of the Daya Bay Experiment and Director of Institute of High Energy Physics, Chinese Academy of Sciences, anno...
History of solar neutrino observations
History of solar neutrino observations
Abstract The first solar neutrino experiment, led by Raymond Davis Jr, showed a deficit of neutrinos relative to the solar model prediction, referred to as the “sola...

Back to Top