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| Main Authors: | , |
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| Format: | Preprint |
| Published: |
2024
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2401.13043 |
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| _version_ | 1866910560634798080 |
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| author | Ansarifard, Saeed Farzan, Yasaman |
| author_facet | Ansarifard, Saeed Farzan, Yasaman |
| contents | The BOREXINO experiment has been collecting solar neutrino data since 2007, providing the opportunity to study the variation of the event rate over a decade. We find that at 96 \% C.L., the rate of low energy events shows a time modulation favoring a correlation with a flux from Jupiter. We present a new physics model, the Jovian Whisper Model, based on dark matter of mass $\sim 0.1-4$ GeV captured by Jupiter that can account for such modulation. We discuss how the Jovian Whisper Model (JWM) can be tested. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2401_13043 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Jovian Signal at BOREXINO Ansarifard, Saeed Farzan, Yasaman High Energy Physics - Phenomenology Earth and Planetary Astrophysics Solar and Stellar Astrophysics The BOREXINO experiment has been collecting solar neutrino data since 2007, providing the opportunity to study the variation of the event rate over a decade. We find that at 96 \% C.L., the rate of low energy events shows a time modulation favoring a correlation with a flux from Jupiter. We present a new physics model, the Jovian Whisper Model, based on dark matter of mass $\sim 0.1-4$ GeV captured by Jupiter that can account for such modulation. We discuss how the Jovian Whisper Model (JWM) can be tested. |
| title | Jovian Signal at BOREXINO |
| topic | High Energy Physics - Phenomenology Earth and Planetary Astrophysics Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2401.13043 |