Effect Of Neutrino Magnetic Moment On Solar Neutrino Observations

2018 ◽  
pp. 338-343
Author(s):  
Arturo Cisneros
1989 ◽  
Vol 04 (02) ◽  
pp. 111-114 ◽  
Author(s):  
PROBHAS RAYCHAUDHURI

It is shown that neutrino flip through the magnetic field of the convection zone is not responsible for the anticorrelation between the solar neutrino flux and the sunspot number.


2005 ◽  
Vol 20 (14) ◽  
pp. 3110-3112 ◽  
Author(s):  
◽  
D. W. Liu

Existence of non-zero neutrino magnetic moment would mean new physics beyond the standard model. A search for the neutrino magnetic moment has been conducted using the high statistic solar neutrino data from Super-Kamiokande-I. This is done by looking for the distortion to the observed energy spectrum of recoil electrons. A non-zero neutrino magnetic moment would cause an increase of event rates at lower energies. The search found no clear signal of neutrino magnetic moment. A limit on the neutrino magnetic moment has been obtained at 3.6 × 10-10μB at 90% C.L. by fitting to the Super-Kamiokande day-night spectra. The effects of neutrino oscillation have been included in the analysis. Including results from other neutrino experiments limiting the oscillation region, a limit of 1.1 × 10-10μB at 90% C.L. was obtained.


1998 ◽  
Vol 57 (3) ◽  
pp. 1794-1800 ◽  
Author(s):  
João Pulido ◽  
Ana M. Mourão

Sign in / Sign up

Export Citation Format

Share Document