Low Metallicity Solar Model Finds the Provement in Borexino Data

The Borexino Collaboration interprets its data within the framework of Bulk Silicate Earth model and the model of the Sun with high metallicity. Other authors have given a different interpretation of the same data within the framework of Hydridic Earth model and low-metallicity Sun model. In order to understand what occasion takes place in Nature, the Borexino single events energy spectrum was numerically simulated using the Monte Carlo method for various assumptions about the processes that could exist in Nature. The existence of large potassium geo-antineutrino flux and its absence were considered. At the same time, the high or low metallicity of the Sun were included in simulations. A comparison of counting rates’ reconstruction from simulated data with the reconstruction of the ones from Borexino single events spectrum demonstrates that large potassium geo-antineutrino flux with low metallicity of the Sun is preferable and is realized in Nature.

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Publication Details

Journal
Physics of Atomic Nuclei
Published
2025-10-01
DOI
https://doi.org/10.1134/s1063778825601581
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
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article

Low Metallicity Solar Model Finds the Provement in Borexino Data

V. V. Sinev, L. B. Bezrukov, A. S. Bykovsky
Physics of Atomic Nuclei
Solar and Space Plasma Dynamics
article

Low Metallicity Solar Model Finds the Provement in Borexino Data

V. V. Sinev, L. B. Bezrukov, A. S. Bykovsky
article en

Abstract

The Borexino Collaboration interprets its data within the framework of Bulk Silicate Earth model and the model of the Sun with high metallicity. Other authors have given a different interpretation of the same data within the framework of Hydridic Earth model and low-metallicity Sun model. In order to understand what occasion takes place in Nature, the Borexino single events energy spectrum was numerically simulated using the Monte Carlo method for various assumptions about the processes that could exist in Nature. The existence of large potassium geo-antineutrino flux and its absence were considered. At the same time, the high or low metallicity of the Sun were included in simulations. A comparison of counting rates’ reconstruction from simulated data with the reconstruction of the ones from Borexino single events spectrum demonstrates that large potassium geo-antineutrino flux with low metallicity of the Sun is preferable and is realized in Nature.

Physics of Atomic NucleiVol. 88(5)
Institute for Nuclear Research (RU), National Research Nuclear University MEPhI (RU)
Openalex Percentile: Top 24%
Solar and Space Plasma Dynamics
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