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Jan , RAL - Walter Winter3 Non-standard neutrino interactions Consider effective four-point interactions Consider effective four-point interactions This leads to a Hamiltonian for propagation: matter potential: This leads to a Hamiltonian for propagation: matter potential: For antineutrinos: H H*, a CC -a CC For antineutrinos: H H*, a CC -a CC
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Optimization of a neutrino factoryOptimization of a neutrino factoryfor non-standard neutrino interactionsfor non-standard neutrino interactions
IDS plenary meetingIDS plenary meetingRAL, United KingdomRAL, United Kingdom
January 16-17, 2008January 16-17, 2008
Walter WinterWalter WinterUniversität WürzburgUniversität Würzburg
Jan. 16-17, 2008 IDS-NF @ RAL - Walter Winter 2
ContentsContents IntroductionIntroduction Our setupOur setup Main questions:Main questions:
– What does the silver channel help?What does the silver channel help?– How small can the muon energy be?How small can the muon energy be?– Standard versus non-standard baseline optimizationStandard versus non-standard baseline optimization
SummarySummary
In collaborationwith Joachim Kopp and
Toshihiko Ota
Jan. 16-17, 2008 IDS-NF @ RAL - Walter Winter 3
Non-standard neutrino interactionsNon-standard neutrino interactions Consider effective four-point interactionsConsider effective four-point interactions
This leads to a Hamiltonian for This leads to a Hamiltonian for propagation: propagation:
matter potential: matter potential:
For antineutrinos: H For antineutrinos: H H*, a H*, aCCCC -a -aCCCC
Jan. 16-17, 2008 IDS-NF @ RAL - Walter Winter 4
NSI constraintsNSI constraints Limits depend Limits depend
on chirality and on chirality and fermionfermion
Neutrino Neutrino propagation in propagation in principle principle sensitive to sensitive to 33uu+3+3dd++ee
We ignore We ignore potential potential production and production and detection effects, detection effects, which can be which can be parameterized parameterized similarly!similarly!
(ISS Physics report, arXiv:0710.4947)
Jan. 16-17, 2008 IDS-NF @ RAL - Walter Winter 5
Relevant parameters for a NFRelevant parameters for a NF
Uninteresting:limited by matter
density uncertainty
Relatively strong constraints
Weak constraints
Complex numbers
Real number
Jan. 16-17, 2008 IDS-NF @ RAL - Walter Winter 6
Our setup: close to IDS baseline!Our setup: close to IDS baseline! Two detectors at Two detectors at
LL11 and L and L22, 50 kt each, 50 kt each 50% E50% E0.50.5 energy resolution energy resolution Backgrounds 0.001/EBackgrounds 0.001/E22
2.5% signal uncertainty, 2.5% signal uncertainty, 20% BG uncertainty20% BG uncertainty
4 yr + 4 yr running time4 yr + 4 yr running time 10102121 useful muon useful muon
decays/year/detector!decays/year/detector! EE=50 GeV, unless stated =50 GeV, unless stated
otherwise otherwise
Old analysis/det.
Our detector
New analysis (diff. L) (Cervera@
Golden 07)
Silver channel:Silver channel:10 kt Silver* from10 kt Silver* fromhep-ph/0606119hep-ph/0606119(Autiero et al ECC with (Autiero et al ECC with 5xSG, 3xBG)5xSG, 3xBG)
Jan. 16-17, 2008 IDS-NF @ RAL - Walter Winter 7
Performance indicators usedPerformance indicators used Definition of Definition of sensitivity similar to sensitivity similar to 1313 sens.: sens.:
Largest fit |Largest fit | which fits a true which fits a true =0 =0 Corresponds to a conservative case discovery Corresponds to a conservative case discovery
potentialpotential All oscillation parameters, NSI phases All oscillation parameters, NSI phases
marginalized over (exceptions: for marginalized over (exceptions: for , which is , which is real, or if real, or if is assumed to be real) is assumed to be real)
Typically only one or two NSI parameters Typically only one or two NSI parameters considered, such as |considered, such as |ee, , , |, |ee---plane-plane
Jan. 16-17, 2008 IDS-NF @ RAL - Walter Winter 8
NSI with magic baselineNSI with magic baseline
Combing the two baselines Combing the two baselines reduces the impact of reduces the impact of correlations drasticallycorrelations drastically(only real (only real ee assumed!) assumed!)
Does one still need the silver Does one still need the silver channel in that case?channel in that case?
3000 km7000 km
Com
bined
arXiv:0709.1980
Close to worst case for degeneracies: CP=3/2, sin2213=0.001
Jan. 16-17, 2008 IDS-NF @ RAL - Walter Winter 9
Correlations at magic baselineCorrelations at magic baseline Including NSI, the magic baseline is not exactly Including NSI, the magic baseline is not exactly
correlation/degeneracy-freecorrelation/degeneracy-free Example: Approximation Example: Approximation
aaCCCC ~ E: ~ E: Standard term drops as 1/EStandard term drops as 1/E44, NSI-Term as 1/E, NSI-Term as 1/E33 High energies important for NSIHigh energies important for NSI!!
Jan. 16-17, 2008 IDS-NF @ RAL - Walter Winter 10
Comparison to our simulation (1)Comparison to our simulation (1)3000 km
7000 kmC
ombined
arXiv:0709.1980Our simulation,
similar setupOur simulation,
our setupOur simulation + our setup,all osc. params marginalized
Only 13 and CP marginalized!
Jan. 16-17, 2008 IDS-NF @ RAL - Walter Winter 11
Comparison to our simulation (2)Comparison to our simulation (2)
3000 km +7000 km
3000 km +7000 km +
Silver*@3000km
3000 km +7000 km +
Disappearance
3000 km + 7000 kmSilver*@3000km +
Disappearance
Disappearance important for , !
Jan. 16-17, 2008 IDS-NF @ RAL - Walter Winter 12
When does the silver channel helpWhen does the silver channel help… in a two baseline setup?… in a two baseline setup?
Assume oneAssume oneNSI parameterNSI parameterat first, such as at first, such as ee
Fix golden Fix golden detectorsdetectors
Where is the Where is the optimaloptimalsilver baseline?silver baseline?
Place Silver* at Place Silver* at golden baseline 1!golden baseline 1!EE >= 50 GeV! >= 50 GeV!
0.01
0.004
Golden detector 1 = Silver baseline
Jan. 16-17, 2008 IDS-NF @ RAL - Walter Winter 13
Minimum muon energy?Minimum muon energy?
Higher muon energy helps; low-E NF not an optionHigher muon energy helps; low-E NF not an option Silver channel: Not relevant for IDS baseline; helps for ESilver channel: Not relevant for IDS baseline; helps for E ~ 50 GeV ~ 50 GeV
IDS baseline?
High-E N
F
IDS baseline?
High-E N
F
Jan. 16-17, 2008 IDS-NF @ RAL - Walter Winter 14
What if more parameters?What if more parameters? Marginalize over phase of Marginalize over phase of ee as well: as well:
Absolute limits: |Absolute limits: || < 0.03, || < 0.03, |ee| < 0.006 (3| < 0.006 (3))Two orders of magnitude improvement of current Two orders of magnitude improvement of current bounds!bounds!
3000km+7000km 3000km+7000km+Silver*@3000km
Jan. 16-17, 2008 IDS-NF @ RAL - Walter Winter 15
Standard versus non-standard Standard versus non-standard optimizationoptimization
Obviously, the main NSI sensitivity comes Obviously, the main NSI sensitivity comes from the golden and disappearance channelsfrom the golden and disappearance channels
Changing the golden baselines will affect Changing the golden baselines will affect the NSI sensitivitiesthe NSI sensitivities
What if there is no silver channel, do the What if there is no silver channel, do the standard and non-standard optimizations standard and non-standard optimizations coincide?coincide?
Perform optimizations in LPerform optimizations in L11-L-L22-space-space
Jan. 16-17, 2008 IDS-NF @ RAL - Walter Winter 16
Standard optimization revisitedStandard optimization revisited All regions:All regions:
Sensitivity for Sensitivity for sinsin22221313>10>10-4.2-4.2 (5(5) for the ) for the shown shown performance performance indicatorindicator
True True CPCP chosen chosen close to worst close to worst casecase
Robust optimum Robust optimum for ~ 4000 + 7500 for ~ 4000 + 7500 kmkm(not <= 3000 (not <= 3000 km!) km!)
Jan. 16-17, 2008 IDS-NF @ RAL - Walter Winter 17
NSI optimization: one parameterNSI optimization: one parameter
Similar to matter effects (which increase with baseline!), Similar to matter effects (which increase with baseline!), NSI sensitivities want one very long baselineNSI sensitivities want one very long baseline
Jan. 16-17, 2008 IDS-NF @ RAL - Walter Winter 18
Combined optimization: ExampleCombined optimization: Example 4000 + 7500 km4000 + 7500 km
consistent withconsistent withNSI optimizationNSI optimization
But: In general,But: In general,choose both choose both baselines rather baselines rather longer than shorter!longer than shorter!
Standard opt: combined
NSI example(CP=/2, sin2213=0.01)
Jan. 16-17, 2008 IDS-NF @ RAL - Walter Winter 19
Summary and conclusionsSummary and conclusions The leading NSI sensitivity comes from the golden + The leading NSI sensitivity comes from the golden +
disappearance channelsdisappearance channels The silver channel might help if EThe silver channel might help if E > 40 GeV > 40 GeV
Return to high-E NF for IDS baseline? Return to high-E NF for IDS baseline? A low-E NF (EA low-E NF (E << 20 GeV) probably has very little NSI << 20 GeV) probably has very little NSI
sensitivity beyond the current limitssensitivity beyond the current limits The currently used IDS baseline setup 4000 km + 7500 The currently used IDS baseline setup 4000 km + 7500
km is consistent for both standard and non-standard km is consistent for both standard and non-standard effects; the baselines be rather longer than shorter!effects; the baselines be rather longer than shorter!
NSI are important to establish the physics case for a very NSI are important to establish the physics case for a very long baselinelong baseline