2013
DOI: 10.1103/physrevlett.111.061803
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Physics Performance of a Low-Luminosity Low Energy Neutrino Factory

Abstract: We investigate the minimal performance, in terms of beam luminosity and detector size, of a neutrino factory to achieve a competitive physics reach for the determination of the mass hierarchy and the discovery of leptonic CP violation. We find that a low luminosity of 2 × 10 20 useful muon decays per year and 5 GeV muon energy aimed at a 10 kton magnetized liquid argon detector placed at 1300 km from the source provides a good starting point. This result relies on θ13 being large and assumes that the so-called… Show more

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Cited by 21 publications
(37 citation statements)
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“…Neutrino oscillation probability depends on various oscillation parameters present in the 3 × 3 mixing matrix -the PMNS matrix [1][2][3] and the neutrino mass squared differences. Two of the three angles -θ 12 and θ 23 present in PMNS matrix have been known with certain accuracy for some time. Recently several experiments like Double CHOOZ, Daya Bay, RENO and T2K collaboration [4][5][6][7] found non-zero value of sin 2 2θ 13 corresponding to the third mixing angle of PMNS matrix with a global level of significance which is well above conventional 5σ discovery threshold.…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…Neutrino oscillation probability depends on various oscillation parameters present in the 3 × 3 mixing matrix -the PMNS matrix [1][2][3] and the neutrino mass squared differences. Two of the three angles -θ 12 and θ 23 present in PMNS matrix have been known with certain accuracy for some time. Recently several experiments like Double CHOOZ, Daya Bay, RENO and T2K collaboration [4][5][6][7] found non-zero value of sin 2 2θ 13 corresponding to the third mixing angle of PMNS matrix with a global level of significance which is well above conventional 5σ discovery threshold.…”
Section: Introductionmentioning
confidence: 99%
“…The mass squared differences -|∆m 2 31 | and ∆m 2 21 is known (where ∆m 2 ij = m 2 i −m 2 j ) but the sign of ∆m 2 31 and as such the hierarchy (whether it is normal (NH) or inverted (IH)) of neutrino masses is still unknown. Various neutrino oscillation experiments like superbeam, neutrino factory, beta beams and reactor experiments are focussing on determining these unknown parameters corresponding to neutrino oscillations [8][9][10][11][12][13][14][15][16][17][18][19].…”
Section: Introductionmentioning
confidence: 99%
“…This constitutes a reduction of luminosity by a factor 5 with respect to the default setup [25]. Then following [270] this permits the detector mass to be reduced from 100 kt to 10 kt. This is but one example of how to achieve this entry level luminosity.…”
Section: B Support Requestmentioning
confidence: 99%
“…The results obtained in [270] for the precision attainable for a measurement of the CP violating phase δ are shown in the left panel of Fig. 119, at 1σ (1 d.o.f.).…”
Section: B Support Requestmentioning
confidence: 99%
“…[40]. More recently, lower energy versions have also been proposed, see for instance [16,41,42], which operate in a regime much closer to the first VOM.…”
Section: Experimental Setupsmentioning
confidence: 99%