A New Sensitive Search for Muon to Electron Conversion Mu2e Experiment at Fermilab Mu2e Collaboration: Boston U, BNL, UC Berkeley & LBNL, UC Irvine, CUNY,

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An accelerator beam of muon neutrinos is manufactured at the Fermi Laboratory in Illinois, USA. The neutrino beam spectrum is sampled by two detectors:
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Presentation transcript:

A New Sensitive Search for Muon to Electron Conversion Mu2e Experiment at Fermilab Mu2e Collaboration: Boston U, BNL, UC Berkeley & LBNL, UC Irvine, CUNY, College of William & Mary, FNAL, JINR, UIUC, INR Troitsk, INFN Lecce, INFN Pisa & U di Pisa, LNF Frascati, UMass Amherst, LANL, Muons Inc, Northwestern U, Rice U, Syracuse U, U of Virginia, U of Washington Lepton Flavor Violation Charged Lepton flavor: accidental symmetry in the Standard Model Lepton flavor violation is forbidden in the Standard Model if neutrinos are massless. A very small SM effect due to finite neutrino mass produces negligibly small rates: BR(   e  ) ~ 10  CLFV: an unambiguous signature of new physics Such small SM rates make charged lepton flavor violation an ideal place to look for new physics, with mass scale sensitivity far beyond the reach of direct searches. The next generation experiments will have sensitivity to directly test predictions of many BSM theories. The Fermilab Mu2e experiment will search for coherent, neutrinoless   e conversion in the field of a nucleus with a sensitivity of 4 orders of magnitude better than existing limits. Mu2e will measure the normalized conversion rate Our goal is to measure R  e with a single-event sensitivity R  e = 2.5  10  History of muon LFV Searches Sensitivity to New Physics Possible New Physics Contributions Randall-Sundrum ~ constrains many models ~ ultimate goal Sensitivity to 10 4 TeV scales: compelling physics case with or without LHC discoveries Required Sensitivity  magnetic moment type operator  → e  rate ~300x  N → eN’ rate  four-fermion interaction  N → eN’ greatly enhanced over  →  e  rate Model independent CLFV Lagrangian: (A. de Gouvea) A. de Gouvea MEGA SINDRUM II MEG goal Mu2e goal ProjectX goal  - N → e - N’ and  + → e +  are Complementary Experimental Technique Negative muons stopped in an Aluminum target form muonic atoms with 1S binding energy of 500 keV and a lifetime of 864 nsec (40% decay, 60% nuclear capture). While the muon and nuclear wavefunctions overlap, the muons can undergo a coherent neutrinoless conversion of a muon to electron: Choice of a nucleus is a tradeoff between higher conversion BR (  with N 2 ), longer lifetime (  with Z 3 ), and higher endpoint energy (N recoil  with N, B.E.  with Z 2 ). Al and Ti have comparable sensitivities. Coherent conversion  N  eN Key Experimental Features:  Pulsed, high-intensity proton beam (2  Hz, 8 Fermilab) with duty cycle matched to muon lifetime.  Solenoidal muon collection and transfer scheme with high acceptance (5  Hz muon rate).  Muons with low momentum and narrow momentum spread to maximize stopping rate and avoid 105 MeV electrons from muon decays in flight.  Excellent momentum resolution for detected electrons, particle ID capabilities. Backgrounds Muon Decays in Orbit Electrons from muon decays in the bound state have an endpoint energy of 105 MeV. The endpoint spectrum falls sharply as This background is minimized by optimizing the electron spectrometer for resolution and reducing multiple scattering. Mu2e goal: FWHM ~0.9 p=105 MeV, with  ~0.3 MeV on the high side. Decay in Orbit electrons ee Simulation with R  e =10 –16 Other Muon-induced Backgrounds Ordinary muon capture on nucleus: Neutral backgrounds produce high-rate environment in the detector. Suppressed by displacing the detectors from the direct line-of-sight from the stopping target and reducing their sensitivity to neutrons and gammas (low-mass gas straw tubes). Proton absorbers downstream of the stopping target reduce charge proton rate. Tracking detectors will also discriminate with dE/dx. Radiative muon capture on nucleus: produces  near conversion energy with probability of O(10 –5 ), can be followed by   e + e – conversion. Endpoint energy for Al is MeV, 2.5 MeV below   e conversion energy. Rate is lower than DIO. Muon decays in flight: suppress contribution to signal region by limiting the muon transport line acceptance to p  <75 MeV. Pions captured on the stopping target emit high-energy photons, which could convert in material and produce an electron in the signal region: Pion stopping rate: 3  10 –7 stopped pions per incident proton. This gives 1.7  10 –13 fake electrons per incident proton. Radiative pion capture is prompt: suppress this background with pulsed beam. Requirements: short (<100 nsec) bunches separated by 1.7  s; 10 –9 proton extinction between bunches. Radiative Pion Capture Backgrounds Cosmic Ray Induced Backgrounds Fake electrons in the region of interest can also be produced by cosmic ray interaction with the detector material and shielding. Suppress these by modest overburden (~6 m of Earth, concrete shielding, magnet yoke steel), pattern recognition in the tracker, and active Cosmic Ray Veto. Summary of Background Contributions SINDRUM-II (current best limit, DC beam) Mu2e Estimates DIO electrons Expect 4   e conversion events for R  e =10 –16 Experimental Apparatus Muons are collected, transported, and detected in superconducting solenoidal magnets. Key features: High acceptance: delivers stopped muons per 8 GeV proton Chicane geometry shields the detector from production target Separation of positive and negative particles, momentum selection Low-mass tracking detector with excellent momentum resolution (  ~0.3 MeV) Production Solenoid Transport Solenoid Selects low momentum   Avoids straight line from production target to detectors Detector Solenoid Proton Target Shielding Muon Beam Collimators Tracker Calorimeter Electrons Muons Muon Stopping Target Proton Beam B=5 T B=1 T B=2 T B=2.5 T B=1 T Based on MECO/MELC design Pions Electromagnetic calorimeter provides robust trigger and particle ID for electrons Cosmic Ray Veto (not shown) rejects cosmic-ray induced background with 99.99% efficiency new detector hall and beamline Minimal accelerator modifications needed: 1.new switch magnet needed to transfer beam from Recycler to Antiproton Accumulator 2.upgrade for 15 Hz Booster rate Proton Beamlines Cycle time determined by Main Injector magnet ramp rate: no NOvA neutrinos lost! Fermilab has a number of rings that become available after the end of the Tevatron operations. The accelerator complex is ideally suited for a broad intensity frontier program. Example: concurrent NOvA and Mu2e beam delivery with minimal accelerator upgrades. Mu2e beam NOvA beam 6 batches x 4x10 12 /1.33 s x 2x10 7 s/yr = 3.6x10 20 protons/yr “Boomerang” scheme ~40x increase in beam power to muon beamline with options for more. Broad scope. Intensity sufficient to reach R  e ~ 10  Will need to upgrade Mu2e to take advantage of the rates Towards 10 –18 Sensitivity: Project X Upgrade path will depend on the results from Mu2e. If a signal is observed at R  e ~10 –  or above, then precision exploration of CLFV mechanisms will require high statistics, and runswith heavier targets (various New Physics couplings scale differently with Z). This will require detector upgrades to handle higher instantaneous rates and shorter muon lifetime. If no signal was seen at Mu2e sensitivity, will improve sensitivity by increasing rates and reducing backgrounds. This will require a redesign of the beamline and detector.