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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN1 Future of Kaon Physics Augusto Ceccucci/CERN J-PARC hypernuclei K Rare Decay U-70 factory Hadron xsec K S decays N ff CERN-SPS Rare K decays LFV Chiral dynamics Frequent K decays
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October 19, 2006 CHIPP BernAugusto Ceccucci/CERN2 CKM Unitarity and Rare Kaon Decays The unitarity of the CKM matrix can be expressed by triangles in a complex plane. There are six triangles, one is more “triangular”: V ud V ub *+V cd V cb *+V td V tb *=0 It is customary to employ the Wolfenstein parameterization: V us ~ V cb ~ V ub ~ i V td ~ i Sensitive to |V td | CP It is important to check that the unitary triangle is the same for all heavy quarks. The s-quark is just as important as the b-quark. If experiment shows that there are differences between the flavors this would be an important discovery.
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October 19, 2006 CHIPP BernAugusto Ceccucci/CERN3 The Global Contest of Flavour and CPV Re ’/ Dm m Bs Sin 2 What will we learn next??
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October 19, 2006 CHIPP BernAugusto Ceccucci/CERN4 Forward Look (Personal Choice) Quantity Exp09 10 11 12 13 14 15 16 Sin2 Peng )~0.05 Belle/Babar Bs )~0.02 LHCb (B DK) LHCb B (s) (SM sens.) LHC (BR(K + ))~ 0.10 P326 (NA48/3) BR(K 0 ) (SM sens.) J-PARC (BR(B Super-B Year: 20XX
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October 19, 2006 CHIPP BernAugusto Ceccucci/CERN5 K→ : SM Theoretical Prediction charm contribution NNLO Buras, Gorbahn, Haisch, Nierste hep-ph/0508165 top contributions NLO Calculation: Buchalla & Buras: 1993, 1999 Misiak, Urban: 1999 The uncertainty of the SM prediction is mostly due to uncertainty of the CKM parameters and not to hadronic matrix elements: BR(K + + ) (1.6×10 -5 )|V cb | 4 [ 2 +( c - ) 2 ] (8.0 ± 1.1)×10 -11 BR(K L 0 ) (7.6×10 -5 )|V cb | 4 2 ± 0.6 ×10 -11
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October 19, 2006 CHIPP BernAugusto Ceccucci/CERN6 MFV: Sensitivity to Z 0 Penguin from Bobeth et a. (2005) 14.4 < q 2 (GeV 2 )< 25 1 < q 2 (GeV 2 ) < 60.04 < q 2 (GeV 2 ) < 1 E > 1.8 GeV
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN7 K 0 L KOPIO @ BNL stopped In Japan a step by step approach is proposed: KEK: –E391a has completed data taking (three runs) –Present limit < 2.1 10 -7 90%CL –Aim to reach the Grossman-Nir bound (~10 -9 ) J-PARC (>2010) –Proposal for the J-PARC hadron facility –Step I: move the improved E391a detector at J-PARC; To reach SM sensitivity Received J-PARC PAC stage I approval –Step II: build a new detector and a dedicated beam-line to be able reach ~ 100 SM events CERN –Evaluating capabilities in the context of an upgraded proton complex
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K 0 L at J-Parc Improvements w.r.t. E391a: CsI calorimeter with a finer granularity New photon veto in the beam Waveform digitization for higher rates
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October 19, 2006 CHIPP BernAugusto Ceccucci/CERN9 K + → + : setting the bar for the next generation of experiments 100 events Mean=SM 100 events Mean=E787/949 Current constraint on plane ? E787/E949: BR(K + → + ) = 1.47 +1.30 -0.89 × 10 -10
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October 19, 2006 CHIPP BernAugusto Ceccucci/CERN10 Plans for K + → + Decays at rest: –There is a Letter of Intent to continue K + → + studies with kaons decays at rest at J-PARC –The plan is to move the BNL-E949 detector to Japan to study Hadron Nuclear Spectroscopy at the Spring-8 LEPS2 photon source –Then, the detector could be moved to J-PARC when/if a low energy K + line becomes available Decays in flight: –Not anymore pursued at FNAL –There is a proposal with a sensitivity to collect about 80 SM events in two years at the CERN-SPS –The proposal (P-326) builds on the infrastructure of the current CERN kaon experiment (NA48/2) and is also known as NA48/3
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN11 Proposal to Measure the Rare Decay K at the CERN SPS CERN, Dubna, Ferrara, Florence, Frascati, Mainz, Merced, Moscow, Naples, Perugia, Protvino, Pisa, Rome, Saclay, San Luis Potosi, Sofia, Turin CERN-SPSC-2005-013 SPSC-P-326 Presented at the CERN SPSC in September 2005 R&D endorsed by CERN Research Board on December 2005 Test beams in Oct-Nov 2006 Seeking more groups to join Aims to complete R&D by the end of 2007…. …to start data taking in 2011
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN12 CERN Proton Complex NA48 SPS LHC CNGS CERN Proton Complex
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN13 NA48
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN14 P-326 Detector Layout SPS primary p: 400 GeV/c Secondary beam: 75 GeV/c 800 MHz /K/p (~6% K + ) K+K+ ++ ~11 MHz of K + decays (KABES) K SPIBES: Si pixel X/X 0 << 1% per station Pixel size ~ 300 x 300 m excellent time resolution
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN 15 Background rejection 1) Kinematical Rejection 2) Photon vetoes to reject K + + 0 : P(K ) = 75 GeV/c Requiring P( ) < 35 GeV/c P( ) > 40 GeV/c It can be hardly missed in the calorimeters!! 3) PID (RICH) for K + + rejection
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN 16 Signal & backgrounds from K decays / year* TotalRegion IRegion II Signal (SM)651649 K++0K++0 2.7±0.21.7±0.21.0±0.1 K2K2 1.2±0.31.1±0.3<0.1 K e4 2±2negligible2±2 K + + and other 3-tracks bckg. 1±1negligible1±1 22 1.3±0.4negligible1.3±0.4 K2K2 0.4±0.10.2±0.1 K e3, K 3,othersnegligible Total bkg9±33.0±0.26±3 SPS used as LHC injector (so it will run in the future) No flagrant time overlap with CNGS P-326 fully compatible with the rest of CERN fixed target Conservative beam request based on decennial NA48 experience at SPS * Before taxes. Proposal quotes a more conservative 40 evt/year @BR=10 -10
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN17 LKr inefficiency measured with data Cluster not reconstructed E = 22 GeV Pion P=42 GeV/c Photon E=11 GeV Expected position track and lower energy are use to predict the position of the other LKr ineff. per (E > 10 GeV): ~ 7 × 10 -6 (preliminary) K + selected kinematically Just collected tagged to measure for E < 10 GeV using an e - beam and the NA48 DCH’s as active target
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN18 Other Physics Opportunities The situation is similar to NA48, which was designed to measure “only” ’/ but produced many more measurements Accumulating ~100 times the flux of NA48/2 will allow us to address, for instance: 1.Cusp like effects ( scattering) –K , K e 2.Lepton Flavour Violation K e , K e +, R K = (K e / K 3.Search for new low mass particles –K X –K P (pseudoscalar sGoldstino) 4.Study rare decays 5.Improve greatly on rare radiative kaon decays 6.Compare K + and K - (alternating beam polarity) –K (CPV interference) –T-odd Correlations in K l4 7.And possibly, given the quality of the detector, topics in hadron spectroscopy Example I Example I I
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN19 Example I: Observation of scattering effect in K→3 decays 1 bin = 0.00015 GeV 2 K ± ± 0 0 4m π + 2 30M events 4m π + 2 NA48/2 has made the first observation the of the charge exchange process + 0 0 in the K 0 0 decay. M 2 ( 0 0 ) (GeV/c 2 ) 2 NA48/2 PLB 633 (2006) hep-ex/0511056 N. Cabibbo, hep-ph/0405001 PRL 93121801 (2004) N. Cabibbo and G. Isidori, hep-ph/0502130 JHEP 503 (2005) G. Colangelo, J. Gasser, et al. hep-ph/0604084 PLB 638 (2006) ~|M 0 +M 1 | 2
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN20 Difference between scattering length in I=0 and I=2 states (a 0 – a 2 )m + = 0.268 ± 0.010(stat) ± 0.004(syst) ± 0.013(theor) In agreement with theory (a 0 – a 2 )m + = 0.265 ± 0.004 (Colangelo 2001) NA48/2 PLB 633 (2006) hep-ex/0511056
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN21 Masiero, Paradisi, Petronzio, hep-ph/0511289 NA48/2 EPS05 EXAMPLE II : R K = (K e ) / (K
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN22 P-326 Project CORE Cost ~26 MCHF –Including about 3.7 MCHF for online/offline computing Cost drivers: –Photon Vetoes: 5.0 MCHF –RICH: 3.0 MCHF –Magnets: 3.0 MCHF –Gigatracker: 2.9 MCHF (0.13 m CMOS) Completion of R&D and TDR submission during 2007 Construction time 2008-2010 –It is a window of opportunity between the completion of the LHC detectors and before the LHC upgrade (SLHC) –A step-by-step upgrade of the to experimental setup allows one to address LFNV and other topics before the full construction of P-326 Data taking with full detector from 2011 The consolidation/upgrade of the CERN proton complex enthuses to also think about an K 0 L
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN23
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN24 Why should CH Participate Outstanding physics opportunity –The importance of rare kaon decays has been recognised by the theoretical community since a long time. If these experiments are not done, we will arguably lack the cleanest test of the SM flavour sector –It is a “no lose situation”. If new particles exists, their effect must appear in loops –No other clean way to study the FCNC d s transitions –Complementary with LHCb –Cost-effective alternative to Super-F factories With a moderate investment CH could play an essential role –The time scale is well matched to bridge the current round of LHC experiments and the ILC/SLHC construction Small risk –The SPS is here to stay and the CERN proton complex will be consolidated –Projects such as this one add breath to the CERN Physics programme low strategic/schedule risk –The experiment is feasible with some more R&D moderate technical risk –The exploitation of existing CERN infrastructure keeps the tag price low low financial risk
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN25 Summary J-PARC –Hypernuclei studies (K1.8 line “day one” experiments) –P14: K L (K0 beam-line, >2010) –P6: Transverse polarisation (K ) (K1.1BR beam-line) –P9: K at rest (>2013) CERN-SPS: P-326 (NA48/3) –K in-flight (Precise SM prediction, Test of MFV) –LFNV: R K = (K e / K , K e -, K e +,… –Chiral dynamics (Ke4, K 4, radiative and non-leptonic kaon decays) – Scattering –Search for new low energy particles –T-odd correlations Other labs (“frequent” decays) –IHEP Protvino (in-flight separated beam) –Frascati factory (hadronic x-sections, K Interferometry, nucleon ff)
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN26 SPARES
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN27 Plans at the Frascati factory Last KLOE run: 2006 DA NE runs until 2008 for other experiments: FINUDA +SIDDHARTA Plans for Luminosity and Energy upgrades (DANAE) CM Energy (GeV) 1.022.4 Peak Luminosity (cm -2 s -1 ) 10 33 10 32 DANAE Motivation: Kaon interferometry (QM) Nuclear Physics N N form factor Synchrotron radiation R&D
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28 Beamline was built in 2001-2004 and commissioned in December 2004 IHEP Protvino: RF-separated beam @U-70 Main beam parameters : Primary proton beam energy 65-70 GeV Primary proton beam intensity 10 13 ppp Secondary beam momentum 12.5 or 18 GeV Length of the beam line ~200m K intensity at the end 5 x 10 6 +, p contamination <25% Muon halo <100 % End of the beamlineDeflector in the beamline
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN29 Expected Backgrounds (J-PARC-Step1) For 7 SM events: S/B~1.4
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN30 P-326 RICH performance P from straws RICH Radiator: STP Ne: (n-1)x10 6 =67.1 L=18 m
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN31 Theory vs. Experiment SM ObservableTheory errorExp error 2006 B(K L ~3%?? B(K ~6%~75% A FB (B X s l l ) ~8%?? B(B X s ) ~10%~9% B(B X s l l ) ~13%~20% A FB (B K ( * ) l l ) ~15%~30% B(B (K ( * ) ) ) ~25%~40% B(B s ) ~30%?? B(B K*l l ) ~35%~13% Adapted from U. Haisch @ Flavour in the LHC era, 6-8 Feb 06, CERN
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN32 Standard Model contribution to P T : P T (SM) < 10 -7 Effects from final state interactions (FSI) : P T (FSI) < 10 -5 A large window for new physics in the region of P T = 10 -3 ~ 10 -5 T-violating Transverse Muon Polarization in K + → Decays P T = - 0.0017 ± 0.0023(stat) ± 0.0011(syst) ( |P T | < 0.0050 : 90% C.L. ) Im = - 0.0053 ± 0.0071(stat) ± 0.0036(syst) ( |Im | <0.016 : 90% C.L. ) KEK-PS E246 result E246 Non-zero P T is a clear signal of T violation
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October 19, 2006 CHIPP Bern Augusto Ceccucci/CERN33 Upgraded E246 experiment at J-PARC Sensitivity goal = P T ~10 -4 P T stat ~ 0.05 P T stat ( E246 ) ~10 -4 P T syst ~ 0.1 P T syst ( E246 ) ~10 -4 Stopped K + decay SC Toroidal spectrometer Active muon polarimeter etc. E246 detector
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