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Near detectors for new physics searches IDS-NF plenary meeting at TIFR, Mumbai October 12, 2009 Walter Winter Universität Würzburg TexPoint fonts used in EMF: AAAAA A A A
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2 Contents Near detectors for standard osc. physics Three (new) physics examples: Non-standard interactions Non-unitarity of the mixing matrix Sterile neutrinos Requirements for new physics searches What we need to understand … NB: For this talk, „near“ means L << 100 km (no std. osc. effect)
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3 Near detectors for standard oscillation physics Need two near detectors, because + / - circulate in different directions For the same reason: if only standard oscillations, no CID required, only excellent flavor-ID Possible locations: (Tang, Winter, arXiv:0903.3039)
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4 Requirements for standard oscillation physics Muon neutrino+antineutrino inclusive CC event rates measured (other flavors not needed in far detectors for IDS-NF baseline) No charge identification, no e, At least same characteristics/quality (energy resolution etc.) as far detectors (a silicon vertex detector or ECC or liquid argon may do much better …) Location and size not really relevant, because extremely large statistics (maybe size relevant for beam monitoring, background extrapolation) The specifications of the near detectors may actually be driven by new physics searches! See my talk tomorrow!
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5 Beam+straight geometry Near detectors described in GLoBES by (E)=A eff /A det x on-axis flux and For (E) ~ 1: Far detector limit Example: OPERA- sized detector at d=1 km: L > ~1 km: GLoBES std. description valid (with L eff ) (Tang, Winter, arXiv:0903.3039)
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6 Effective operator picture if mediators integrated out: Describes additions to the SM in a gauge-inv. way! Example: TeV-scale new physics d=6: ~ (100 GeV/1 TeV) 2 ~ 10 -2 compared to the SM d=8: ~ (100 GeV/1 TeV) 4 ~ 10 -4 compared to the SM Interesting dimension six operators Fermion-mediated Non-unitarity (NU) Scalar or vector mediated Non-standard int. (NSI) New physics from heavy mediators mass d=6, 8, 10,...: NSI, NU
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7 Example 1: Non-standard interactions Typically described by effective four fermion interactions (here with leptons) May lead to matter NSI (for = =e) May also lead to source/detector NSI (e.g. NuFact: s for = =e, = ) These source/det.NSI are process-dep.!
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8 Lepton flavor violation … and the story of SU(2) gauge invariance Strong bounds ee e NSI (FCNC) ee e CLFV e 4 -NSI (FCNC) Ex.: e e Affects neutrino oscillations in matter (or neutrino production) Affects environments with high densities (supernovae) BUT: These phenomena are connected by SU(2) gauge invariance Difficult to construct large leptonic matter NSI with d=6 operators (Bergmann, Grossman, Pierce, hep-ph/9909390; Antusch, Baumann, Fernandez-Martinez, arXiv:0807.1003; Gavela, Hernandez, Ota, Winter,arXiv:0809.3451) Need d=8 effective operators, …! Finding a model with large NSI is not trivial!
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9 On current NSI bounds (Source NSI for NuFact) The bounds for the d=6 (e.g. scalar-mediated) operators are strong (CLFV, Lept. univ., etc.) (Antusch, Baumann, Fernandez-Martinez, arXiv:0807.1003) The model-independent bounds are much weaker (Biggio, Blennow, Fernandez-Martinez, arXiv:0907.0097) However: note that here the NSI have to come from d=8 (or loop d=6?) operators ~ (v/ ) 4 ~ 10 -4 natural? „NSI hierarchy problem“?
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10 Source NSI with at a NuFact Probably most interesting for near detectors: e s, s (no intrinsic beam BG) Near detectors measure zero-distance effect ~ | s | 2 Helps to resolve correlations (Tang, Winter, arXiv:0903.3039) ND5: OPERA-like ND at d=1 km, 90% CL This correlation is always present if: - NSI from d=6 operators - No CLFV (Gavela et al, arXiv:0809.3451; see also Schwetz, Ohlsson, Zhang, arXiv:0909.0455 for a particular model)
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11 Other types of source NSI In particular models, also other source NSI (without detection) are interesting Example: (incoh.) e s from addl. Higgs triplet as seesaw (II) mediator 1 kt, 90% CL, perfect CID (Malinsky, Ohlsson, Zhang, arXiv:0811.3346) Requires CID! Geometric effects? Effects of std. oscillations Systematics (CID) limitation? CID important!
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12 Example 2: Non-unitarity of mixing matrix Integrating out heavy fermion fields, one obtains neutrino mass and the d=6 operator (here: fermion singletts) Re-diagonalizing and re-normalizing the kinetic terms of the neutrinos, one has This can be described by an effective (non-unitary) mixing matrix with N=(1+ ) U Similar effect to NSI, but source, detector, and matter NSI are correlated in a particular, fundamental way (i.e., process- independent) also: „MUV“
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13 Impact of near detector Example: (Antusch, Blennow, Fernandez-Martinez, Lopez-Pavon, arXiv:0903.3986) near detector important to detect zero-distance effect Magnetization not mandatory, size matters Curves: 10kt, 1 kt, 100 t, no ND
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14 Example 3: Search for sterile neutrinos 3+n schemes of neutrinos include (light) sterile states The mixing with the active states must be small The effects on different oscillation channels depend on the model test all possible two-flavor short baseline (SBL) cases, which are standard oscillation-free Example: e disappearance Some fits indicate an inconsistency between the neutrino and antineutrino data (see e.g. Giunti, Laveder, arXiv:0902.1992) NB: Averaging over decay straight not possible! The decays from different sections contribute differently!
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15 SBL e disappearance Averaging over straight important (dashed versus solid curves) Location matters: Depends on m 31 2 Magnetic field if interesting as well (Giunti, Laveder, Winter, arXiv:0907.5487) 90% CL, 2 d.o.f., No systematics, m=200 kg Two baseline setup? d=50 m d~2 km (as long as possible)
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16 SBL systematics Systematics similar to reactor experiments: Use two detectors to cancel X-Sec errors (Giunti, Laveder, Winter, arXiv:0907.5487) 10% shape error arXiv:0907.3145 Also possible with only two ND (if CPT-inv. assumed)
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17 CPTV discovery reaches (3 ) (Giunti, Laveder, Winter, arXiv:0907.5487) Dashed curves: without averaging over straight Requires four NDs!
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18 Summary of (new) physics requirements Number of sites At least two (neutrinos and antineutrinos), for some applications four (systematics cancellation) Exact baselines Not relevant for source NSI, NU, important for oscillatory effects (sterile neutrinos etc.) Flavors All flavors should be measured Charge identification Is needed for some applications (such as particular source NSI); the sensitivity is limited by the CID capabilities Energy resolution Probably of secondary importance (as long as as good as FD); one reason: extension of straight leads already to averaging Detector size In principle, as large as possible. In practice, limitations by beam geometry or systematics. Detector geometry As long (and cylindrical) as possible (active volume) A eff < A det A eff ~ A det
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19 What we need to understand How long can the baseline be for geometric reasons (maybe: use „alternative locations“)? What is the impact of systematics (such as X-Sec errors) on new physics parameters What other kind of potentially interesting physics with oscillatory SBL behavior is there? How complementary or competitive is a near detector to a superbeam version, see e.g. http://www-off-axis.fnal.gov/MINSIS/
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