Javascript must be enabled to continue!
Standard Model Tested with Neutrinos
View through CrossRef
The standard model (SM) of particle physics effectively explains most observed phenomena, though some anomalies, especially in the neutrino sector, suggest the need for extensions. In this Letter, we perform the first global fit of elastic neutrino-nucleus and neutrino-electron scattering data to further test the SM within a consistent framework. Our results on the neutrino charge radius, the only nonzero electromagnetic property of neutrinos in the SM, show no significant deviation, indicating no large beyond the SM flavor-dependent effects for electron and muon neutrinos. By incorporating solar neutrino data from dark matter direct detection experiments, we also place the most stringent constraints on the tau neutrino charge radius obtained from neutrino scattering experiments. Additionally, we determine updated constraints on the vector and axial-vector neutrino-electron neutral current couplings, adjusting for flavor-dependent effects and for the different experimental momentum transfers. The global analysis reveals two allowed solutions: one close to the SM prediction, and a degenerate solution that is favored. We show that future dark matter detectors could achieve sufficient precision to resolve the degeneracy. As we move toward the precision era, this Letter demonstrates the crucial need to properly account for flavor- and momentum-dependent effects to avoid misinterpretations of the data.
American Physical Society (APS)
Title: Standard Model Tested with Neutrinos
Description:
The standard model (SM) of particle physics effectively explains most observed phenomena, though some anomalies, especially in the neutrino sector, suggest the need for extensions.
In this Letter, we perform the first global fit of elastic neutrino-nucleus and neutrino-electron scattering data to further test the SM within a consistent framework.
Our results on the neutrino charge radius, the only nonzero electromagnetic property of neutrinos in the SM, show no significant deviation, indicating no large beyond the SM flavor-dependent effects for electron and muon neutrinos.
By incorporating solar neutrino data from dark matter direct detection experiments, we also place the most stringent constraints on the tau neutrino charge radius obtained from neutrino scattering experiments.
Additionally, we determine updated constraints on the vector and axial-vector neutrino-electron neutral current couplings, adjusting for flavor-dependent effects and for the different experimental momentum transfers.
The global analysis reveals two allowed solutions: one close to the SM prediction, and a degenerate solution that is favored.
We show that future dark matter detectors could achieve sufficient precision to resolve the degeneracy.
As we move toward the precision era, this Letter demonstrates the crucial need to properly account for flavor- and momentum-dependent effects to avoid misinterpretations of the data.
Related Results
From T2K to Hyper-Kamiokande : neutrino oscillation analysis and preparation of the time synchronization system
From T2K to Hyper-Kamiokande : neutrino oscillation analysis and preparation of the time synchronization system
De T2K à Hyper-Kamiokande : analyse d’oscillation des neutrinos et préparation du système de synchronisation en temps
Les neutrinos sont les particules du Modèle St...
Etude des oscillations de neutrinos atmosphériques avec le télescope à neutrinos ANTARES
Etude des oscillations de neutrinos atmosphériques avec le télescope à neutrinos ANTARES
Les neutrinos sont probablement les particules les plus particulières connues à ce jours. Dès la première hypothèse sur leur existence, en 1930, jusqu'à aujourd'hui, ils ont incité...
Interacciones de neutrinos: efectos colectivos y aplicaciones a medios astrofísicos
Interacciones de neutrinos: efectos colectivos y aplicaciones a medios astrofísicos
La astrofísica teórica en la actualidad se basa en la conjunción de modelos electrodébiles, la física de hadrones y bariones, y modelos de estructuras extendidas de la materia. Un ...
Recherche de neutrinos lourds avec l'expérience T2K
Recherche de neutrinos lourds avec l'expérience T2K
La masse non-nulle des neutrinos rend nécessaire l'introduction de nouvelle physique pour expliquer celle-ci. Par exemple, l'ajout de neutrinos lourds avec une masse de l'ordre du ...
A common origin for the QCD axion and sterile neutrinos from SU(5) strong dynamics
A common origin for the QCD axion and sterile neutrinos from SU(5) strong dynamics
Abstract
We identify the QCD axion and right-handed (sterile) neutrinos as bound states of an SU(5) chiral gauge theory with Peccei-Quinn (PQ) symmetry arising...
Multi-messenger observations with the KM3NeT telescope : search for high energy neutrinos coinciding with fast radio transients
Multi-messenger observations with the KM3NeT telescope : search for high energy neutrinos coinciding with fast radio transients
Observations multi-messagers avec le télescope à neutrinos KM3NeT : recherche de neutrinos de haute énergie en coïncidence avec des transitoires radio rapides
À l’è...
Detecting and studying high-energy collider neutrinos with FASER at the LHC
Detecting and studying high-energy collider neutrinos with FASER at the LHC
AbstractNeutrinos are copiously produced at particle colliders, but no collider neutrino has ever been detected. Colliders produce both neutrinos and anti-neutrinos of all flavors ...
Heavy Neutrinos at Large Colliders
Heavy Neutrinos at Large Colliders
Abstract
In this work we discuss the state of the art of the heavy neutrinos at colliders. The neutrinos in the Standard Model (SM) are considered to be massless whi...

