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@ARTICLE{Appel:916130,
author = {Appel, S. and Bagdasarian, Z. and Basilico, D. and Bellini,
G. and Benziger, J. and Biondi, R. and Caccianiga, B. and
Calaprice, F. and Caminata, A. and Cavalcante, P. and
Chepurnov, A. and D’Angelo, D. and Derbin, A. and Di
Giacinto, A. and Di Marcello, V. and Ding, X. F. and Di
Ludovico, A. and Di Noto, L. and Drachnev, I. and Franco, D.
and Galbiati, C. and Ghiano, C. and Giammarchi, M. and
Goretti, A. and Göttel, A. S. and Gromov, M. and Guffanti,
D. and Ianni, Aldo and Ianni, Andrea and Jany, A. and
Kobychev, V. and Korga, G. and Kumaran, S. and Laubenstein,
M. and Litvinovich, E. and Lombardi, P. and Lomskaya, I. and
Ludhova, L. and Lukyanchenko, G. and Machulin, I. and
Martyn, J. and Meroni, E. and Miramonti, L. and Misiaszek,
M. and Muratova, V. and Nugmanov, R. and Oberauer, L. and
Orekhov, V. and Ortica, F. and Pallavicini, M. and Papp, L.
and Pelicci, L. and Penek, Ö. and Pietrofaccia, L. and
Pilipenko, N. and Pocar, A. and Raikov, G. and Ranalli, M.
T. and Ranucci, G. and Razeto, A. and Re, A. and Redchuk, M.
and Rossi, N. and Schönert, S. and Semenov, D. and
Settanta, G. and Skorokhvatov, M. and Singhal, A. and
Smirnov, O. and Sotnikov, A. and Tartaglia, R. and Testera,
G. and Unzhakov, E. and Villante, F. L. and Vishneva, A. and
Vogelaar, R. B. and von Feilitzsch, F. and Wojcik, M. and
Wurm, M. and Zavatarelli, S. and Zuber, K. and Zuzel, G.},
title = {{I}mproved {M}easurement of {S}olar {N}eutrinos from the
{C}arbon-{N}itrogen-{O}xygen {C}ycle by {B}orexino and {I}ts
{I}mplications for the {S}tandard {S}olar {M}odel},
journal = {Physical review letters},
volume = {129},
number = {25},
issn = {0031-9007},
address = {College Park, Md.},
publisher = {APS},
reportid = {FZJ-2022-05959},
pages = {252701},
year = {2022},
abstract = {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.},
cin = {IKP-2},
ddc = {530},
cid = {I:(DE-Juel1)IKP-2-20111104},
pnm = {612 - Cosmic Matter in the Laboratory (POF4-612)},
pid = {G:(DE-HGF)POF4-612},
typ = {PUB:(DE-HGF)16},
pubmed = {36608219},
UT = {WOS:001005991200001},
doi = {10.1103/PhysRevLett.129.252701},
url = {https://juser.fz-juelich.de/record/916130},
}