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@ARTICLE{Appel:912318,
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 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 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 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 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. and
Rossi, N.},
title = {{I}ndependent determination of the {E}arth’s orbital
parameters with solar neutrinos in {B}orexino},
journal = {Astroparticle physics},
volume = {145},
number = {0927-6505},
issn = {0927-6505},
address = {Amsterdam [u.a.]},
publisher = {Elsevier Science},
reportid = {FZJ-2022-05510},
pages = {102778},
year = {2023},
abstract = {Since the beginning of 2012, the Borexino collaboration has
been reporting precision measurements of the solar neutrino
fluxes, emitted in the proton–proton chain and in the
Carbon–Nitrogen–Oxygen cycle. The experimental
sensitivity achieved in Phase-II and Phase-III of the
Borexino data taking made it possible to detect the annual
modulation of the solar neutrino interaction rate due to the
eccentricity of Earth’s orbit, with a statistical
significance greater than 5. This is the first precise
measurement of the Earth’s orbital parameters based solely
on solar neutrinos and an additional signature of the solar
origin of the Borexino signal. The complete periodogram of
the time series of the Borexino solar neutrino detection
rate is also reported, exploring frequencies between one
cycle/year and one cycle/day. No other significant
modulation frequencies are found. The present results were
uniquely made possible by Borexino’s decade-long
high-precision solar neutrino detection.},
cin = {IKP-2},
ddc = {540},
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},
UT = {WOS:000873805900001},
doi = {10.1016/j.astropartphys.2022.102778},
url = {https://juser.fz-juelich.de/record/912318},
}