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Future Fermilab Flavor Physics Program

Future Fermilab Flavor Physics Program. Brendan Casey , Fermilab , FPCP2011. Probing the highest energies. p. New Physics Energy Scale, L NP. 10 13 TeV. n seesaw . K +. p. m. K L. 10 3 TeV. n m. LHC compositeness . 1 TeV. n m ,n e. Current Rings/Accelerators.

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Future Fermilab Flavor Physics Program

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  1. Future Fermilab Flavor Physics Program Brendan Casey , Fermilab, FPCP2011

  2. Probing the highest energies p New Physics Energy Scale, LNP 1013 TeV n seesaw K+ p m KL 103 TeV nm LHC compositeness 1TeV nm ,ne B. Casey, FPCP 2011

  3. Current Rings/Accelerators Main Injector 150 GeV Accumulator & Debuncher 8 GeV Booster 8 GeV Tevatron LINAC 400 MeV Recycler 8 GeV Cockcroft-Walton 750 keV NuMI BooNE B. Casey, FPCP 2011

  4. Upgrades for experiments this decade Major proton source accelerator improvement project for increased beam power and reliability for next 15 years of operation Booster: 7 Hz  15 Hz 2x flux @ 8 GeV Main Injector 150 GeV Accumulator & Debuncher 8 GeV Booster 8 GeV K+ LINAC 400 MeV p Recycler 8 GeV Mu2e 200 MHz RFQ NuMI BooNE LBNE MI: 400 kW 700 kW @ 120 GeV g-2 Next generation muon, Kaon, and neutrino experiments B. Casey, FPCP 2011

  5. Upgrades for Experiments next decade g-2, mEDM LBNE Short baseline n experiments > 2 MW @ 60-80 GeV ~3 MW high duty factor @ 3 GeV 1 GeV available mNeN mEDM meg, eee m+e-m-e+ Rare isotopes, EDMs Nuclear energy and waste transmutation test facility K+ K0 B. Casey, FPCP 2011

  6. Neutrino Beamlines n factory ??? + upgrades Local MiniBooNE MicroBooNE MINERvA SBNE South Dakota wide band 1300k LBNE + upgrades Minnesota on axis 735 km MINOS + upgrades Minnesota off axis 810km NOvA + upgrades B. Casey, FPCP 2011

  7. Leptogenesis GUT Murayama hep-ph/0208005 EW Need to know q13 0nbb expectations PMNS Need to know mass hierarchy n2 n3 n1 Dm2> 0 Dm2< 0 n2 n3 n1 • “Archeological evidence:” • No electroweak baryogenesis • CPV in light, left n • Lepton number violation • What info do we need to do these experiments? B. Casey, FPCP 2011

  8. NOvA Effective mass n2 ne n1 n3 Dm2< 0 Dm2> 0 n2 n1 n3 Oscillation frequency increases or decreases depending on hierarchy ne Far detector Building May 18 Antineutrino interaction in surface prototype Ash River 4/18/2011 B. Casey, FPCP 2011

  9. LBNE • Broad physics program • Oscillations • Astrophysics • Proton decay • Scope of each will depend on detector choice B. Casey, FPCP 2011 • Longer baseline • 8101300km • Larger detector • 2 x 100 kt Water • 2 x 17 kt Liquid Ar • Next generation q13, CPV experiments

  10. n-factory n factory Ultimate and perhaps necessary reach comes from muon storage ring Variations on LBNE 4 MW p, 5 GeV m MuCool test area at Fermilab. First beam delivered Feb 2011 Project X Muonacceleration program (MAP) formed to unify US funded R&D and prove feasibility of muon collider in the next few years B. Casey, FPCP 2011

  11. And much more Address anomalies with MicroBooNE, MINOS+ Precision cross section measurements with MINERvA Ambitious LAr R&D program ArgoNeuT mBooNE B. Casey, FPCP 2011

  12. Antiprotons World’s greatest antimatter factory Charm, hyperon, exotics 2.6 nanograms last year Anti Hydrogen Anti Gravity Will be repurposed for muon production but there is still interesting physics that may be unique to this facility B. Casey, FPCP 2011

  13. Kaons Same motivation for FCNC B and K programs d s s b Difference is the size of the SM ‘background’ B mesons: Vts l2 orVtd l3 or Vub l3 Kaons: Vts*Vtd  l5 Generic couplings: Kaons win, flavor specific: need both B. Casey, FPCP 2011

  14. K+p+nn 1st 2nd 3rd generation at BNL = 7 event data sample BNL E787 event display Can get hundreds of evts per year starting with beam from Main Injector and continuing with Project X B. Casey, FPCP 2011

  15. K0p0nn Pico-bunches Pointing Pencil beam Plus a lot more 200 evt/yr possible with Project X Generic couplings: Kaons win, flavor specific: need both B. Casey, FPCP 2011

  16. Other Kaon measurements Enormous data sets + multipurpose detectors = lots of physics B. Casey, FPCP 2011

  17. Charged lepton flavor program An observation of charged lepton flavor violation expected in the next decade implies existence of a new mixing matrix. Expect same as quarks, neutrinos: multi-decade program to determine 4 parameters of the matrix Cold traps, intense muon sources, super B factories, t/charm factories, lepton colliders, Hadron colliders… m→eg, mN→eN t→eg, eee t→mg, mmm (g-2)e, (g-2)m, (g-2)t CP violation: lepton EDM measurements B. Casey, FPCP 2011

  18. G-2 Pbar complex target ring B. Casey, FPCP 2011 • Follow up of BNL experiment but better: • Reuse the storage ring • 10x longer decay channel • Segmented calorimeters • Tracking • >20x statistics, >2x less systematics • Coupled with a world wide program to interpret the measurement

  19. Mu2e Direct conversion of a muon into an electron Diagrams in common with meg Diagrams not accessible to meg bkg signal Mu2e goal: 3 x10-17wrt capture (LNP~104TeV) B. Casey, FPCP 2011

  20. m  e with Project X Option 1: LFV established  design for precision measurements / properties Option 2: LFV not established  design for maximum sensitivity 3 x 10-19 possible with Project X beam power Conversion rate vrs target Z Vector current dipole Scalar current B. Casey, FPCP 2011

  21. EDMs MFV + 1 new phase + Bs CPV = EDM Large Bs CPV shrinks available parameter space 10-25 EDMs this decade ?!?! Thallium 10-30 neutron Mercury Bs CPV Buras, Isidori, Paradisi arXiv:1007.5291 B. Casey, FPCP 2011

  22. EDMs B EDM=0 w S E m rest frame B w S EDM≠0 E • e EDM: • Can amplify signal using high Z Alkali metals • Outer electron is in s-wave: size of electron becomes size of atom. • Factor ~1000 enhancement for Francium • Project X nuclear physics facility: copious production of desired heavy isotopes • m EDM: • EDM tilts precession plane of muons in a storage ring • Factor 100 improvement possible with New g-2 experiment • Extra factor 10000 possible with dedicated storage ring in Project X muon facility B. Casey, FPCP 2011

  23. Near term timeline B. Casey, FPCP 2011

  24. Conclusions p K+ p m KL nm nm ,ne B. Casey, FPCP 2011 • Fermilab is planning a diverse neutrino and targeted rare process program that covers many of the most important low energy observables • In several cases, Fermilab is the best place to perform these experiments • Beam power + duty factor • In many, it is the only place to perform these measurements to high precision due to unique features of Project X • The program will play an integral role in interpreting LHC results, will push the envelope in precision detector technology, and will provide unique opportunities to grad students and post docs.

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