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| Hauptseite > Publikationsdatenbank > Improved Measurement of Solar Neutrinos from the Carbon-Nitrogen-Oxygen Cycle by Borexino and Its Implications for the Standard Solar Model > print |
| Hauptseite > Publikationsdatenbank > Improved Measurement of Solar Neutrinos from the Carbon-Nitrogen-Oxygen Cycle by Borexino and Its Implications for the Standard Solar Model > print |
| 001 | 916130 | ||
| 005 | 20230814101441.0 | ||
| 024 | 7 | _ | |a 10.1103/PhysRevLett.129.252701 |2 doi |
| 024 | 7 | _ | |a 0031-9007 |2 ISSN |
| 024 | 7 | _ | |a 1079-7114 |2 ISSN |
| 024 | 7 | _ | |a 1092-0145 |2 ISSN |
| 024 | 7 | _ | |a 2128/33232 |2 Handle |
| 024 | 7 | _ | |a 36608219 |2 pmid |
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| 037 | _ | _ | |a FZJ-2022-05959 |
| 082 | _ | _ | |a 530 |
| 100 | 1 | _ | |a Appel, S. |0 P:(DE-HGF)0 |b 0 |
| 245 | _ | _ | |a Improved Measurement of Solar Neutrinos from the Carbon-Nitrogen-Oxygen Cycle by Borexino and Its Implications for the Standard Solar Model |
| 260 | _ | _ | |a College Park, Md. |c 2022 |b APS |
| 336 | 7 | _ | |a article |2 DRIVER |
| 336 | 7 | _ | |a Output Types/Journal article |2 DataCite |
| 336 | 7 | _ | |a Journal Article |b journal |m journal |0 PUB:(DE-HGF)16 |s 1671620327_30681 |2 PUB:(DE-HGF) |
| 336 | 7 | _ | |a ARTICLE |2 BibTeX |
| 336 | 7 | _ | |a JOURNAL_ARTICLE |2 ORCID |
| 336 | 7 | _ | |a Journal Article |0 0 |2 EndNote |
| 520 | _ | _ | |a We present an improved measurement of the carbon-nitrogen-oxygen (CNO) solar neutrino interaction rate at Earth obtained with the complete Borexino Phase-III dataset. The measured rate, RCNO=6.7+2.0−0.8 counts/(day×100 tonnes), allows us to exclude the absence of the CNO signal with about 7σ C.L. The correspondent CNO neutrino flux is 6.6+2.0−0.9×108 cm−2 s−1, taking into account the neutrino flavor conversion. We use the new CNO measurement to evaluate the C and N abundances in the Sun with respect to the H abundance for the first time with solar neutrinos. Our result of NCN=(5.78+1.86−1.00)×10−4 displays a ∼2σ tension with the “low-metallicity” spectroscopic photospheric measurements. Furthermore, our result used together with the 7Be and 8B solar neutrino fluxes, also measured by Borexino, permits us to disfavor at 3.1σ C.L. the “low-metallicity” standard solar model B16-AGSS09met as an alternative to the “high-metallicity” standard solar model B16-GS98. |
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| 773 | _ | _ | |a 10.1103/PhysRevLett.129.252701 |g Vol. 129, no. 25, p. 252701 |0 PERI:(DE-600)1472655-5 |n 25 |p 252701 |t Physical review letters |v 129 |y 2022 |x 0031-9007 |
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