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Constraints on Flavor-Diagonal Non-Standard Neutrino Interactions from Borexino Phase-II

Authors :
G. Korga
D. Jeschke
Z. Bagdasarian
S. Appel
E. Litvinovich
K. Fomenko
Michael Wurm
M. Gschwender
Matthias Laubenstein
B. Caccianiga
Ö. Penek
F. Calaprice
Sanjib Kumar Agarwalla
J. Thurn
L. Lukyanchenko
J. Martyn
F. Gabriele
D. Bick
Sandra Zavatarelli
G. Raikov
Livia Ludhova
A. M. Goretti
A. S. Chepurnov
Tatsu Takeuchi
O. Zaimidoroga
E. Meroni
G. Zuzel
Cristiano Galbiati
P. Cavalcante
Gioacchino Ranucci
B. Neumair
D. Guffanti
M. Nieslony
D. Bravo
Fausto Ortica
G. Lukyanchenko
G. Testera
Tobias Lachenmaier
Marco Giammarchi
G. Bellini
A. Sotnikov
R. Tartaglia
N. Rossi
D. Semenov
Kai Zuber
Aldo Ianni
S. Kumaran
E. V. Unzhakov
Xuefeng Ding
A. Vishneva
A. Di Ludovico
Matteo Agostini
D. Franco
J. Maricic
Andrey Formozov
D. Basilico
M. Skorokhvatov
N. Pilipenko
F. von Feilitzsch
Y. Suvorov
S. Rottenanger
L. Oberauer
V. N. Muratova
Caren Hagner
M. Gromov
M. Meyer
Andrea Ianni
A. Di Giacinto
A. Razeto
G. Manuzio
I. N. Machulin
A. V. Derbin
M. Misiaszek
Marco Pallavicini
D. D'Angelo
C. Ghiano
A. Jany
L. Cappelli
L. Pietrofaccia
A. Pocar
Marcin Wójcik
V. Atroshchenko
Chen Sun
M. Redchuk
Paolo Lombardi
Lino Miramonti
V. Di Marcello
V. V. Kobychev
E. Hungerford
I. Drachnev
F. Cavanna
K. Altenmüller
R. B. Vogelaar
Alessandra Re
A. Caminata
V. Orekhov
S. Marcocci
G. Bonfini
J. Benziger
K. Choi
S. Davini
Aldo Romani
L. Papp
L. Di Noto
Oleg Smirnov
Stefan Schönert
Agarwalla, S. K.
Agostini, M.
Altenmuller, K.
Appel, S.
Atroshchenko, V.
Bagdasarian, Z.
Basilico, D.
Bellini, G.
Benziger, J.
Bick, D.
Bonfini, G.
Bravo, D.
Caccianiga, B.
Calaprice, F.
Caminata, A.
Cappelli, L.
Cavalcante, P.
Cavanna, F.
Chepurnov, A.
Choi, K.
D'Angelo, D.
Davini, S.
Derbin, A.
Di Giacinto, A.
Di Marcello, V.
Ding, X. F.
Di Ludovico, A.
Di Noto, L.
Drachnev, I.
Fomenko, K.
Formozov, A.
Franco, D.
Gabriele, F.
Galbiati, C.
Gschwender, M.
Ghiano, C.
Giammarchi, M.
Goretti, A.
Gromov, M.
Guffanti, D.
Hagner, C.
Hungerford, E.
Ianni, A.
Jany, A.
Jeschke, D.
Kumaran, S.
Kobychev, V.
Korga, G.
Lachenmaier, T.
Laubenstein, M.
Litvinovich, E.
Lombardi, P.
Ludhova, L.
Lukyanchenko, G.
Lukyanchenko, L.
Machulin, I.
Manuzio, G.
Marcocci, S.
Maricic, J.
Martyn, J.
Meroni, E.
Meyer, M.
Miramonti, L.
Misiaszek, M.
Muratova, V.
Neumair, B.
Nieslony, M.
Oberauer, L.
Orekhov, V.
Ortica, F.
Pallavicini, M.
Papp, L.
Penek, O.
Pietrofaccia, L.
Pilipenko, N.
Pocar, A.
Raikov, G.
Ranucci, G.
Razeto, A.
Re, A.
Redchuk, M.
Romani, A.
Rossi, N.
Rottenanger, S.
Schonert, S.
Semenov, D.
Skorokhvatov, M.
Smirnov, O.
Sotnikov, A.
Sun, C.
Suvorov, Y.
Takeuchi, T.
Tartaglia, R.
Testera, G.
Thurn, J.
Unzhakov, E.
Vishneva, A.
Vogelaar, R. B.
von Feilitzsch, F.
Wojcik, M.
Wurm, M.
Zaimidoroga, O.
Zavatarelli, S.
Zuber, K.
Zuzel, G.
Agarwalla, S
Agostini, M
Altenmuller, K
Appel, S
Atroshchenko, V
Bagdasarian, Z
Basilico, D
Bellini, G
Benziger, J
Bick, D
Bonfini, G
Bravo, D
Caccianiga, B
Calaprice, F
Caminata, A
Cappelli, L
Cavalcante, P
Cavanna, F
Chepurnov, A
Choi, K
D'Angelo, D
Davini, S
Derbin, A
Di Giacinto, A
Di Marcello, V
Ding, X
Di Ludovico, A
Di Noto, L
Drachnev, I
Fomenko, K
Formozov, A
Franco, D
Gabriele, F
Galbiati, C
Gschwender, M
Ghiano, C
Giammarchi, M
Goretti, A
Gromov, M
Guffanti, D
Hagner, C
Hungerford, E
Ianni, A
Jany, A
Jeschke, D
Kumaran, S
Kobychev, V
Korga, G
Lachenmaier, T
Laubenstein, M
Litvinovich, E
Lombardi, P
Ludhova, L
Lukyanchenko, G
Lukyanchenko, L
Machulin, I
Manuzio, G
Marcocci, S
Maricic, J
Martyn, J
Meroni, E
Meyer, M
Miramonti, L
Misiaszek, M
Muratova, V
Neumair, B
Nieslony, M
Oberauer, L
Orekhov, V
Ortica, F
Pallavicini, M
Papp, L
Penek, O
Pietrofaccia, L
Pilipenko, N
Pocar, A
Raikov, G
Ranucci, G
Razeto, A
Re, A
Redchuk, M
Romani, A
Rossi, N
Rottenanger, S
Schonert, S
Semenov, D
Skorokhvatov, M
Smirnov, O
Sotnikov, A
Sun, C
Suvorov, Y
Takeuchi, T
Tartaglia, R
Testera, G
Thurn, J
Unzhakov, E
Vishneva, A
Vogelaar, R
von Feilitzsch, F
Wojcik, M
Wurm, M
Zaimidoroga, O
Zavatarelli, S
Zuber, K
Zuzel, G
AstroParticule et Cosmologie (APC (UMR_7164))
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)
Borexino
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris
PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)
Observatoire de Paris
PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Physics
Source :
JHEP, JHEP, 2020, 02, pp.038. ⟨10.1007/JHEP02(2020)038⟩, Journal of High Energy Physics, Journal of High Energy Physics, 2020, 02, pp.038. ⟨10.1007/JHEP02(2020)038⟩, Journal of high energy physics 2020(2), 38 (2020). doi:10.1007/JHEP02(2020)038, Journal of High Energy Physics, Vol 2020, Iss 2, Pp 1-29 (2020), Journal of high energy physics : JHEP 2020(2), 38 (2020). doi:10.1007/JHEP02(2020)038
Publication Year :
2019
Publisher :
arXiv, 2019.

Abstract

The Borexino detector measures solar neutrino fluxes via neutrino-electron elastic scattering. Observed spectra are determined by the solar-$\nu_{e}$ survival probability $P_{ee}(E)$, and the chiral couplings of the neutrino and electron. Some theories of physics beyond the Standard Model postulate the existence of Non-Standard Interactions (NSI's) which modify the chiral couplings and $P_{ee}(E)$. In this paper, we search for such NSI's, in particular, flavor-diagonal neutral current interactions that modify the $\nu_e e$ and $\nu_\tau e$ couplings using Borexino Phase II data. Standard Solar Model predictions of the solar neutrino fluxes for both high- and low-metallicity assumptions are considered. No indication of new physics is found at the level of sensitivity of the detector and constraints on the parameters of the NSI's are placed. In addition, with the same dataset the value of $\sin^2\theta_W$ is obtained with a precision comparable to that achieved in reactor antineutrino experiments.<br />Comment: 28 pages, 7 figures. Slight modifications in the title, abstract, and conclusion. Few references added. Text expanded for clarity. Accepted in JHEP

Subjects

Subjects :
Physics - Instrumentation and Detectors
neutrino: solar
Physics::Instrumentation and Detectors
Solar neutrino
Physics beyond the Standard Model
Electron
metal: solar
01 natural sciences
neutrino: flux
High Energy Physics - Experiment
High Energy Physics - Experiment (hep-ex)
High Energy Physics - Phenomenology (hep-ph)
solar [model]
elastic scattering [neutrino electron]
[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]
neutrino/e: coupling
detector [neutrino]
Borexino
Physics
Elastic scattering
interaction [neutrino/tau]
new physics
Beyond Standard Model
Neutrino Physics
Instrumentation and Detectors (physics.ins-det)
neutrino electron: elastic scattering
coupling [neutrino/e]
nuclear reactor [antineutrino]
High Energy Physics - Phenomenology
neutrino: detector
Astrophysics - Solar and Stellar Astrophysics
coupling [neutrino]
solar [neutrino]
Neutrino
precision measurement [Weinberg angle]
model: solar
Nuclear and High Energy Physics
Particle physics
sensitivity [detector]
FOS: Physical sciences
neutrino/tau: interaction
neutral current: coupling
Weinberg angle: precision measurement
neutrino: new interaction
neutrino: spectrum
0103 physical sciences
antineutrino: nuclear reactor
neutrino: coupling
lcsh:Nuclear and particle physics. Atomic energy. Radioactivity
ddc:530
010306 general physics
Solar and Stellar Astrophysics (astro-ph.SR)
Standard solar model
chiral [coupling]
Neutral current
010308 nuclear & particles physics
solar [metal]
High Energy Physics::Phenomenology
coupling [neutral current]
spectrum [neutrino]
flux [neutrino]
coupling: chiral
detector: sensitivity
new interaction [neutrino]
[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]
lcsh:QC770-798
High Energy Physics::Experiment
Neutrino Physic

Details

ISSN :
11266708 and 10298479
Database :
OpenAIRE
Journal :
JHEP, JHEP, 2020, 02, pp.038. ⟨10.1007/JHEP02(2020)038⟩, Journal of High Energy Physics, Journal of High Energy Physics, 2020, 02, pp.038. ⟨10.1007/JHEP02(2020)038⟩, Journal of high energy physics 2020(2), 38 (2020). doi:10.1007/JHEP02(2020)038, Journal of High Energy Physics, Vol 2020, Iss 2, Pp 1-29 (2020), Journal of high energy physics : JHEP 2020(2), 38 (2020). doi:10.1007/JHEP02(2020)038
Accession number :
edsair.doi.dedup.....f5941cc96e6813e3efe6b560a28c1bb7
Full Text :
https://doi.org/10.48550/arxiv.1905.03512