An independent search for Jovian neutrinos using BOREXINO data
arXiv:2506.14506 · doi:10.1088/1475-7516/2025/12/021
Abstract
In a recent study, arXiv:2401.13043 found evidence for a 6% flux contribution from Jupiter to the total flux rate time series data from the BOREXINO solar neutrino experiment, specifically during the time intervals 2019-2021 and 2011-2013. The significance of this detection was estimated to be around . We reanalyze the BOREXINO data and independently confirm the Jovian signal with the same amplitude and significance as that obtained in arXiv:2401.13043. However, using the same technique, we also find a spurious flux contribution from Venus and Saturn (at significance), whereas prima facie one should not expect any signal from any other planet. We then implement Bayesian model comparison to ascertain whether the BOREXINO data contain an additional contribution from Jupiter, Venus or Saturn. We find Bayes factors of less than five for an additional contribution from Jupiter, and less than or close to one for Venus and Saturn. This implies that the evidence for an additional contribution from Jupiter is very marginal.
33 pages, 20 figures. Accepted for publication in JCAP
References in corpus (7)
- The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package
- Markov Chain Monte Carlo Methods for Bayesian Data Analysis in Astronomy
- Profile Likelihoods in Cosmology: When, Why and How illustrated with CDM, Massive Neutrinos and Dark Energy
- On Model Selection in Cosmology
- Independent determination of the Earth's orbital parameters with solar neutrinos in Borexino
- Constraints on Lorentz Invariance Violation from Gamma-ray Burst rest-frame spectral lags using Profile Likelihood
- Determination of Hubble constant from Megamaser Cosmology Project using Profile Likelihood