Sterile neutrinos at the CNGS

dc.creatorDonini, A.
dc.creatorMaltoni, M.
dc.creatorMeloni, D.
dc.creatorMigliozzi, P.
dc.creatorTerranova, F.
dc.date2007-04-03
dc.date2007-10-11
dc.date.accessioned2026-07-07T12:23:51Z
dc.date.available2026-07-07T12:23:51Z
dc.descriptionWe study the potential of the CNGS beam in constraining the parameter space of a model with one sterile neutrino separated from three active ones by an $\mathcal{O}(\eVq)$ mass-squared difference, $\Dmq_\Sbl$. We perform our analysis using the OPERA detector as a reference (our analysis can be upgraded including a detailed simulation of the ICARUS detector). We point out that the channel with the largest potential to constrain the sterile neutrino parameter space at the CNGS beam is $ν_μ\to ν_τ$. The reason for that is twofold: first, the active-sterile mixing angle that governs this oscillation is the less constrained by present experiments; second, this is the signal for which both OPERA and ICARUS have been designed, and thus benefits from an extremely low background. In our analysis we also took into account $ν_μ\to ν_e$ oscillations. We find that the CNGS potential to look for sterile neutrinos is limited with nominal intensity of the beam, but it is significantly enhanced with a factor 2 to 10 increase in the neutrino flux. Data from both channels allow us, in this case, to constrain further the four-neutrino model parameter space. Our results hold for any value of $\Dmq_\Sbl \gtrsim 0.1 \eVq$, \textit{i.e.} when oscillations driven by this mass-squared difference are averaged. We have also checked that the bound on $θ_{13}$ that can be put at the CNGS is not affected by the possible existence of sterile neutrinos.
dc.descriptionMajor modifications; new analysis after MiniBooNE data release: 21 pages, 5 figures
dc.identifierhttps://arxiv.org/abs/0704.0388
dc.identifierhttp://arxiv.org/abs/0704.0388
dc.identifierJHEP 0712:013,2007
dc.identifierdoi:10.1088/1126-6708/2007/12/013
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/214136
dc.subjectHigh Energy Physics - Phenomenology
dc.titleSterile neutrinos at the CNGS
dc.typetext

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