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Solar Neutrino Physics with Borexino
by Andrea Pocar
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Submission summary
| Authors (as registered SciPost users): | Andrea Pocar |
| Submission information | |
|---|---|
| Preprint Link: | https://arxiv.org/abs/1810.12967v2 (pdf) |
| Date accepted: | Jan. 15, 2019 |
| Date submitted: | Dec. 31, 2018, 1 a.m. |
| Submitted by: | Andrea Pocar |
| Submitted to: | SciPost Physics Proceedings |
| Proceedings issue: | The 15th International Workshop on Tau Lepton Physics (TAU2018) |
| Ontological classification | |
|---|---|
| Academic field: | Physics |
| Specialties: |
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| Approach: | Experimental |
Abstract
We present the most recent solar neutrino results from the Borexino experiment at the Gran Sasso underground laboratory. In particular, refined measurements of all neutrinos produced in the {\it pp} fusion chain have been made. It is the first time that the same detector measures the entire range of solar neutrinos at once. These new data weakly favor a high-metallicity Sun. Prospects for measuring CNO solar neutrinos are also discussed.
Author comments upon resubmission
v2 has a few stylistic fixes
Published as SciPost Phys. Proc. 1, 025 (2019)