Neutrino Factory Physics Study Plots
Kerrys Plot Area
Rajas Plot Area
Superbeams draft report
Steves Talk
at the 2 day meeting for the neutrino factory
physics study, 17-18 Feb, 2000.
sin2 2theta(13) reach summary plot
Superbeam plots
Fig. 3 for superbeams paper
Very long baseline conventional beam setup at FNAL
Decay channel length versus baseline for conventional beams at FNAL
Pion decay fraction versus baseline for conventional beams at FNAL
Superbeam sin**2 2theta(13) sensitivity vs E and L: Rate table for WBB, LAr
Superbeam sin**2 2theta(13) sensitivity vs E and L: Rate table for NBB, water
C
NUMI medium energy beam, baseline 2800 km, s2 2theta(13) = 0.01
NUMI medium energy beam, baseline 2800 km, s2 2theta(13) = 0.04
Draft paper
Figures for entry level and beyond paper
Fig. X1
Wrong-sign muon CC interaction spectrum versus muon threshold energy.
Fig. X2
sin**2 2theta(13) reach for 10 nue->numu event observation vs L and dm(32)**2.
Fig. X3
Thresholds of interest summary plot
Fig. X4
sin**2 2theta(13) reach for 3 sigma sign of dm(32)**2 vs L with E = 20 GeV.
Fig. X5
sin**2 2theta(13) reach for 3 sigma sign of dm(32)**2 vs L and E.
Fig. X6
sin**2 2theta(13) reach for 3 sigma for
(a) delta = 0 vs +pi/2 with dm**2 positive,
(b) delta = 0 vs +pi/2 with dm**2 negative,
(c)delta = 0 vs -pi/2 with dm**2 positive, and
(d) delta = 0 vs -pi/2 with dm**2 negative.
vs L and E for 10**21 decays and a 50 kt detector.
Fig. X8
Tau appearance event rates versus sin**2 2 theta(13) and delta m**2(32)
for E = 20 GeV, L = 2800 km.
Fig. X9
sin**2 2 theta(13) reach for 10 nue -> nutau events versus baseline and
energy.
Getting ready for short baseline paper
nue - nutau / nebar -> nutau bar for scenario IB1
(LSND+ATMOS)
and numu -> nutau / numubar -> nutau bar rates versus delta
-> Fig. 1 of paper. Normalization for error bars is a 1 kt
detector, 3 years running, 10**20 decays/yr, 30 percent efficiency.
nue - nutau for scenario IB1
(LSND+ATMOS)
and numu -> nutau CC rates versus delta.
Other plots
Fig.16
sin**2 2theta(13) reach for CP sensitivity versus L and Emu
Fig.15
Wrong-sign muon CC interaction spectrum versus muon threshold energy.
Fig.14
Sin**2 2theta(13)for 3 sig sign delta m**2 vs Emu and Baseline
- parameter point IA1. Emin = 4 GeV, M = 50 kt. 10**20 decays.
Fig.13
Physics interest versus muon energy and intensity:
summary plot for three-flavor oscillation scenario.
Fig.12
nu(e) -> nu(tau) appearance rates versus delta
for Emu = 20 GeV, L = 60 km
- parameter point IB1 (3-flavor, LSND + Atmos.)
Fig.11
Tau appearance rates versus baseline and stored mu- energy,
for delta = 0 and 90 deg
- parameter point IB1 (3-flavor, LSND + Atmos.)
Fig.10
Tau appearance rates versus baseline and stored mu+ energy,
for delta = 0 and 90 deg
- parameter point IB1 (3-flavor, LSND + Atmos.)
Fig.9
Relative wrong-sign mu rates versus baseline for delta = 0 and 90 deg
- parameter point IA1 with dm**2 = 0.002, 0.005 eV**2 and
Emu = 20 GeV, Emin = 4 GeV.
Fig.8
Sin**2 2theta(13)for 10 events vs dm**2 and Baseline
- parameter point IA1. Emu = 20 GeV, Emin = 4 GeV.
Fig.7
Total CC rate (no oscillations) vs baseline
- Emu = 20 GeV, 50 kt detector, 10**19 decays.
Fig.6
Sin**2 2theta(13)for 3 sig sign delta m**2 vs dm**2 and Baseline
- parameter point IA1. Emu = 20 GeV, Emin = 4 GeV, M = 50 kt. 10**20 decays.
Fig.5
Sin**2 2theta(13)for 10 events vs dm**2 and Emin
- parameter point IA1. Emu = 20 GeV, L = 732 km.
Fig.4
Sin**2 2theta(13)for 10 events vs dm**2 and Emin
- parameter point IA1. Emu = 20 GeV, L = 7332 km.
Fig.3
Minimum Sin**2 2theta(13) - parameter point IA1
Fig.2
Minimum Sin**2 2theta(13) - parameter point IA2
Fig.1
Minimum Sin**2 2theta(13) - parameter point IA3
HIMUS99 workshop writeup
Last updated 9th Jan, 2000
S. Geer sgeer@fnal.gov