Generalized Lomb-Scargle Analysis of 22 years of Super-Kamiokande solar B neutrino data
arXiv:2402.11258 · doi:10.1140/epjc/s10052-024-12846-y
Abstract
We apply the generalized Lomb-Scargle periodogram to 22 years data of solar B neutrino fluxes detected by Super-Kamiokande. The primary motivation of this work was to check if the sinusoidal modulation at a frequency of 9.43/year (with a period of 38 days), which we had found to be marginally significant with the first five years of Super-K data, persists, with the accumulated data. We use four different metrics for the calculation of significance. We do not find any evidence for periodicity at the aforementioned frequency or any other frequency with the updated data. Therefore the marginally detected periodicity at 9.43/year with the first five years of data was only a statistical fluctuation.
arXiv comment8 pages, 3 figures. Accepted for publication in EPJC
References in corpus (10)
- Evidence for oscillation of atmospheric neutrinos
- The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package
- Measurement of the solar neutrino energy spectrum using neutrino-electron scattering
- Search for Dark Matter WIMPs using Upward Through-going Muons in Super-Kamiokande
- Introduction to astroML: Machine Learning for Astrophysics
- Solar neutrino oscillations and bounds on neutrino magnetic moment and solar magnetic field
- A search for periodic modulations of the solar neutrino flux in Super-Kamiokande-I
- Power-Spectrum Analyses of Super-Kamiokande Solar Neutrino Data: Variability and its Implications for Solar Physics and Neutrino Physics
- Likelihood scan of the Super-Kamiokande I time series data
- Evidence for R-Mode Oscillations in Super-Kamiokande Solar Neutrino Data