Download presentation
Presentation is loading. Please wait.
Published byGabriel Marshall Modified over 9 years ago
1
Oscillation Neutrino Physics Reach at Neutrino Factories M. Lindner Technical University Munich
2
M. LindnerNuFact042 Motivation for Precision surprise! how small? spectrum? Dirac and Majorana CP phases? neutrino masses are physics beyond the Standard Model new window to flavour problem – see-saw amplified! information complimentary to quarks:
3
M. LindnerNuFact043 Guessing the Neutrino Mass Spectrum quarks hierarchical masses neutrinos? large mixings! inversely correlated hierarchy in M R ? non-hierarchical, type II see-saw,.... ? Quarks and charged leptons: m D ~ H n ; n = 0,1,2 H > 20... 200 Neutrinos: m ~ H n 1< H < 10 See-saw: 1 20 ? >20 m = -m D T M R -1 m D
4
M. LindnerNuFact044 The Value of Precision for 13 for example: sin 2 2 13 < 0.01 physics question: small 13 numerical coincidence systematic (symmetry,...) how small? precision! models for masses & mixings input: Known masses & mixings distribution of 13 „predictions“ 13 often close to experimental bounds motivates new experiments 13 controls 3-flavour effects like CP-violation
5
M. LindnerNuFact045 mass spectrum, mixings, CP-phases, LVF, 0 2 decay,... Standard Model extensionsflavour symmetries leptogenesis mechanisms supernovae nucleosynthesis structure formation... renormalization group The Interplay of different Topics -parameters extremely valuable long term: most precise flavour info
6
M. LindnerNuFact046 x. The Future of Oscillations
7
M. LindnerNuFact047 2 flavour approximation: P ab = sin 2 (2 sin 2 ( m 2 L/4E) P aa = 1 - P ab Oscillation Channels MSW + parameter mapping
8
M. LindnerNuFact048 Analytical Description analytic discussion / full numerical simulations degeneracies, correlations,... (sin 2 2 13 ) eff
9
M. LindnerNuFact049 running: K2K establish / test atm. osc. with beams construction: MINOS (2005) ~ 10% for m 31 2, 23, improve 13 CNGS: ICARUS & OPERA (2006) approval: T2K (JHF-SK) (2008) few% for m 31 2, 23, improve 13 LOIs: NO A (NuMI-OA) (200x) H2K (JHF-HK) (201x) % for m 31 2, 23, 13, CP, sgn( m 2 ) long term: beams, neutrino factory,... (201x) precision.....muon collider.... every stage is a necessary prerequisit for the next continuous line of improvements for beams, detectors, physics!. Long Baseline: Projects and Plans (partly) precision neutrino physics
10
M. LindnerNuFact0410 Beams conventional beams / superbeams -beams neutrino factories other: laser driven?...?
11
M. LindnerNuFact0411 Determination of the Physics Potential select a setup (beam, detector, baseline,...) take „most realistic“ parameters best guess! simulate all relevant aspects as good as possible GLoBES determine the potential: „true“ fitted parameters consider other options, time, cost, improvements,... compare only realistic simulations discuss the reliability of the input (assumptions) think of improvements R&D in all directions until decisions must be made
12
M. LindnerNuFact0412 Sensitivitiy Plots limit for (sin 2 2 13 ) eff sin 2 2 13 systematics correlationsdegeneracies statistical limit (all parameters fixed) limit for sin 2 2 13 from *THIS* experiment only precise knowledge of some parameter combination = precision of the experiment synergies = combine with other experiments gain more than statistics
13
M. LindnerNuFact0413. 13 Sensitiviy: Comparison of the coming Generation
14
M. LindnerNuFact0414 Adding a new reactor experiment identical detectors many errors cancel
15
M. LindnerNuFact0415. 13 Sensitiviy: Comparison of the next Generation Huber, ML, Rolinec, Schwetz, Winter
16
M. LindnerNuFact0416 Leptonic CP-Violation: Best Case today: sin 2 2 13 < 0.2 assume: sin 2 2 13 = 0.1 and combine: T2K + NO A + Reactor limits or signs of leptonic CP violation Huber, ML, Rolinec, Schwetz, Winter
17
M. LindnerNuFact0417 Neutrino Factory: I & II define benchmark neutrino factories: magnetized iron detector wrong sign ‘s baseline 3000km P(MW) ‘s/year T +T (y) M(kt) -------------------------------------------------------------------------------- Neutrino factory I: 0.75 10 20 5 10 Neutrino factroy II: 4.00 5.3*10 20 8 50 _ simulations of various options: Barger, Geer, Raja, Whisnant, Marfatia,... Cervera, Donini, Gavela, Gomez-Cadenaz, Hernandez, Mena, Rigolin,... Bueno, Campanelli, Rubbia,... Minakata, Yasuda,... Freund, Huber, ML, Winter,......
18
M. LindnerNuFact0418 different sensitivity reductions by systematics correlations & degeneracies lead to severe sensitivity reductions break C&D by combining different experiments of comparable potential T2K NO A
19
M. LindnerNuFact0419.
20
M. LindnerNuFact0420 Measurement of CP Violation
21
M. LindnerNuFact0421 Various Potential Options Initially rate driven improve by combination of different E and/or L or „magic baseline“ combination of different channels or experiments use energy spectrum superbeams: E ≈ GeV large low Z sampling calorimeters ≈ 50 kt superbeams, -beams: E ≈GeV huge Cerenkov detectors ≈ 1000 t huge liquid Ar detectors ≈ 100 kt huge scintillator detectors ≈ 30 kt neutrino factory: E ≈20-50 GeV large magnetized iron Calorimeters ≈ 40kt large magnetized liquid Ar detectors ≈20kt large OPERA-like emulsion detectors ≈5kt laser driven acceleration, …
22
M. LindnerNuFact0422 Combining: Silver Channels Donini, Meloni, Migliozzi Autiero, et al. golden channel: wrong sign ‘s silver channel : ‘s different oscillation probabilities break degeneracies!
23
M. LindnerNuFact0423 Energy Resolution =+ /2 =0 = - /2 rate based degeneracies have different energy spectra 730km use energy resolution to break degeneracies A. Rubbia
24
M. LindnerNuFact0424 A Powerful Simulation Tool General Long Baseline Experiment Simulator P. Huber, ML, W. Winter see parallel talk! http://www.ph.tum.de/~globes hep-ph/0407xxx Release: Aug. 1, 2004 C-based simulation software (GPL – free, for Unix systems) extensive documentation & examples 3 phase approach: experiment definition with AEDL ( Abstract Experiment Definition Language ) simulation of an experiment 3- oscillations; scan „true values“ analysis event distriutions,...., sensitivities,...
25
M. LindnerNuFact0425 Abstract Experiment Definition Language (AEDL) predefined AEDL files for a number of experiments allows easy modifications of „default“ experiments
26
M. LindnerNuFact0426 AEDL Description of a Neutrino Factory !%GLoBES /* beam */ flux(#mu_plus)< @builtin = 1 @parent_energy = 50.0 @stored_muons = 5.33e+20 @time = 8.0 > $target_mass = 50 $bins = 20 $emin = 4.0 $emax = 50.0 /* cross section */ cross(#CC)< @cross_file = XCC.dat > /* baseline */ $baseline = 3000.0 $densitytab = {3.5} $lengthtab = {3000.0} $density_error = 0.05 /* energy resolution */ energy(#MINOS)< @type = 1 @sigma_e = {0.15,0.0,0.0} /* channels */ channel(#appearance)< @channel = #mu_plus: +: electron: muon: #CC: #MINOS > channel(#disappearance)< @channel = #mu_plus: -: muon: muon: #CC: #MINOS > /* rules */ rule(#rule1)< @signal = 0.45 @ #appearance @signalerror = 0.001 : 0.0001 @background = 1.0e-05 @ #disappearance @backgroundcenter = 1 : 0.0 @backgrounderror = 0.05 : 0.0001 @errordim = 0 @energy_window = 4.0 : 50.0 >
27
M. LindnerNuFact0427 GLoBES Simulations sin 2
28
M. LindnerNuFact0428 MINOS, ICARUS and OPERA - improve leading oscillation parameters; should improve sin 2 2 13 a little T2K, NO A and new reactor experiments - further improved leading oscillation parameters - will improve sin 2 2 13 by about one order of magnitude - with luck: sign( m 2 ) or even CP phase H2K, -beams, neutrino factory - can do all unless sin 2 2 13 is extremely tiny; in any case precision -physics! very precise 3- oscillation parameters sin 2 2 13, sign( m 2 ) and CP phase should be measured unique impact on model building! R&D for -beams, neutrino factories... realistic parameters simulate & compare GLoBES http://www.ph.tum.de/~globes and hep-ph/0407xxx Conclusions
Similar presentations
© 2025 SlidePlayer.com. Inc.
All rights reserved.