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000916130 0247_ $$2doi$$a10.1103/PhysRevLett.129.252701
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000916130 1001_ $$0P:(DE-HGF)0$$aAppel, S.$$b0
000916130 245__ $$aImproved Measurement of Solar Neutrinos from the Carbon-Nitrogen-Oxygen Cycle by Borexino and Its Implications for the Standard Solar Model
000916130 260__ $$aCollege Park, Md.$$bAPS$$c2022
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000916130 520__ $$aWe 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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000916130 7001_ $$0P:(DE-HGF)0$$aBellini, G.$$b3
000916130 7001_ $$0P:(DE-HGF)0$$aBenziger, J.$$b4
000916130 7001_ $$0P:(DE-HGF)0$$aBiondi, R.$$b5
000916130 7001_ $$0P:(DE-HGF)0$$aCaccianiga, B.$$b6
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000916130 7001_ $$0P:(DE-HGF)0$$aCavalcante, P.$$b9
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000916130 7001_ $$0P:(DE-HGF)0$$aDi Marcello, V.$$b14
000916130 7001_ $$0P:(DE-HGF)0$$aDing, X. F.$$b15
000916130 7001_ $$0P:(DE-HGF)0$$aDi Ludovico, A.$$b16
000916130 7001_ $$0P:(DE-HGF)0$$aDi Noto, L.$$b17
000916130 7001_ $$0P:(DE-HGF)0$$aDrachnev, I.$$b18
000916130 7001_ $$0P:(DE-HGF)0$$aFranco, D.$$b19
000916130 7001_ $$0P:(DE-HGF)0$$aGalbiati, C.$$b20
000916130 7001_ $$0P:(DE-HGF)0$$aGhiano, C.$$b21
000916130 7001_ $$0P:(DE-HGF)0$$aGiammarchi, M.$$b22
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000916130 7001_ $$0P:(DE-HGF)0$$aIanni, Aldo$$b27
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000916130 7001_ $$0P:(DE-HGF)0$$aLomskaya, I.$$b36
000916130 7001_ $$0P:(DE-Juel1)168122$$aLudhova, L.$$b37$$eCorresponding author$$ufzj
000916130 7001_ $$0P:(DE-HGF)0$$aLukyanchenko, G.$$b38
000916130 7001_ $$0P:(DE-HGF)0$$aMachulin, I.$$b39
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000916130 7001_ $$0P:(DE-HGF)0$$aOrtica, F.$$b48
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000916130 7001_ $$0P:(DE-Juel1)186943$$aPelicci, L.$$b51$$ufzj
000916130 7001_ $$0P:(DE-Juel1)171602$$aPenek, Ö.$$b52$$ufzj
000916130 7001_ $$0P:(DE-HGF)0$$aPietrofaccia, L.$$b53
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000916130 7001_ $$0P:(DE-HGF)0$$aPocar, A.$$b55
000916130 7001_ $$0P:(DE-HGF)0$$aRaikov, G.$$b56
000916130 7001_ $$0P:(DE-HGF)0$$aRanalli, M. T.$$b57
000916130 7001_ $$0P:(DE-HGF)0$$aRanucci, G.$$b58
000916130 7001_ $$0P:(DE-HGF)0$$aRazeto, A.$$b59
000916130 7001_ $$0P:(DE-HGF)0$$aRe, A.$$b60
000916130 7001_ $$0P:(DE-Juel1)171322$$aRedchuk, M.$$b61
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000916130 7001_ $$0P:(DE-Juel1)180506$$aSettanta, G.$$b65
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000916130 7001_ $$0P:(DE-HGF)0$$aVillante, F. L.$$b73
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000916130 7001_ $$0P:(DE-HGF)0$$aVogelaar, R. B.$$b75
000916130 7001_ $$0P:(DE-HGF)0$$avon Feilitzsch, F.$$b76
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000916130 773__ $$0PERI:(DE-600)1472655-5$$a10.1103/PhysRevLett.129.252701$$gVol. 129, no. 25, p. 252701$$n25$$p252701$$tPhysical review letters$$v129$$x0031-9007$$y2022
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