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PRISM/PRIME Overview Yoshitaka Kuno Department of Physics Osaka - PowerPoint PPT Presentation

PRISM/PRIME Overview Yoshitaka Kuno Department of Physics Osaka University November 8th, 2010 Project-X Muon Workshop PRISM/`PRIME Option PRISM/PRIME Detector Layout Aiming at a single event sensitivity of 3x10 -19 PRISM/PRIME Detector


  1. PRISM/PRIME Overview Yoshitaka Kuno Department of Physics Osaka University November 8th, 2010 Project-X Muon Workshop

  2. PRISM/`PRIME Option

  3. PRISM/PRIME Detector Layout Aiming at a single event sensitivity of 3x10 -19

  4. PRISM/PRIME Detector Layout PRIME detector PRISM-FFAG muon storage ring PRISM beamline

  5. What is a Muon to Electron Conversion ? 1s state in a muonic atom Neutrino-less muon nuclear capture (= μ -e conversion) nucleus − + ( A , Z ) → e − + ( A , Z ) µ µ − lepton flavors muon decay in orbit changes by one unit. − → e − νν µ nuclear muon capture − N ) = Γ ( µ − N → e − N ) − N → e − + ( A , Z ) → ν µ + ( A , Z − 1) B ( µ µ ' ) − N → ν N Γ ( µ

  6. Search for μ -e Conversion is like .... meditation (since no complicated analysis). But make sure you are ready in advance.

  7. Potential Background for μ -e Conversion • Background rejection is the most important in searches for rare decays. • Types of backgrounds for μ - +N → e - +N are, • muon decay in orbit originate from muons Intrinsic • radiative muon capture stopping in the muon backgrounds • muon capture with particle emission stopping target. • radiative pion capture • muon decay in flight caused by beam particles, • pion decay in flight Beam-related such as electrons, pions, • beam electrons backgrounds muons, and anti-protons • neutron induced in a beam • antiproton induced • cosmic-ray induced Other • room-background induced anything others backgrounds • pattern recognition error

  8. Previous Measurements Published Results (2004) SINDRUM-II (PSI) B ( µ − + Au → e − + Au ) < 7 × 10 − 13 1m A exit beam solenoid F inner drift chamber B gold target G outer drift chamber C vacuum wall H superconducting coil Class 1 events: prompt forward removed D scintillator hodoscope I helium bath J E Cerenkov hodoscope J magnet yoke e - measurement I H 10 3 e + measurement G F MIO simulation D D E H C 10 2 A µ e simulation B events / channel 10 configuration 2000 1 SINDRUM II 80 90 100 Class 2 events: prompt forward PSI muon beam intensity ~ 10 7-8 /sec beam from the PSI cyclotron. To eliminate 10 beam related background from a beam, a 1 beam veto counter was placed. But, it could not work at a high rate. 80 90 100 momentum (MeV/c)

  9. Improvements for Background Rejection at Mu2e and COMET at 10 -16 Beam pulsing with measured Beam-related between beam separation of 1 μ sec backgrounds pulses proton extinction = #protons between pulses/#protons in a pulse < 10 -9 low-mass trackers in improve Muon DIO electron energy vacuum & thin target background resolution curved solenoids for eliminate Muon DIF energetic muons momentum selection background (>75 MeV/c) base on the MELC proposal at Moscow Meson Factory

  10. Why Mu2e and COMET cannot go beyond ? • (1) Beam background rejection is heavily relined on proton beam extinction of 10 -9 , which is uncertain. • (2) The beam line is not long enough, so that late pions might come in a beam. • The measurement starts after 700 nsec after the prompt. • Material of a muon stopping target is limited to low Z.

  11. PRISM Beamline

  12. PRISM (Phase Rotated Intense Slow Muon source) momentum slit PRISM-FFAG extract kickers muon storage ring matching section PRISM curved solenoid beamline (short) SC solenoid / pulsed horns injection kickers

  13. PRISM to reject beam-related backgrounds (1) • (1) Rejection of pions in a beam (like radiative π capture) most • long flight length of a beam important • use a muon storage ring • in PRISM, a circumference of the PRISM FFAG muon storage ring is about 40 meters, and 5-6 turns would give about 200 meters. • then, pion survival rate is < 10 -20 . • alternative is a long solenoid, but very expensive..... • (2) Rejection of beam particles with wrong momenta from upstream • dipole magnet and momentum slits before a muon stopping target • very narrow momentum slit allowing only 40 MeV/c +- 3% • no 100 MeV particles coming in (such as muon decay inflight) • selecting of muons that would stop in a muon-stopping target • no beam dump needed and no flush

  14. PRISM to reject beam-related backgrounds (2) • The curved-solenoid momentum selection may not be sharp enough for 10 -18 • (3) Beam extinction at both proton and muon beams • (injection) kicker magnets for the storage ring does this for muons, • in addition to proton beam extinction • a total beam extinction of 10 -11 • (4) Narrow muon beam energy spread • allow a thinner muon stopping target (1/10 of Mu2E and COMET) • by phase rotation in a muon storage ring • goal is +- 3% from +-30 % • This is not a critical issue, since we can make tight momentum selection of the signal electron (just a loss of acceptance).

  15. PRISM to reject cosmic/exp. hall backgrounds • (1) Rejection of cosmic-induced or neutrons/gammas-induced backgrounds • low duty factor running might help.....

  16. PRISM Specifications • Intensity : • 40 MeV/c ±3% • 2x10 12 muons/sec. • at extraction of the muon • for multi-MW proton beam storage ring. power • Central Momentum : ���������������� • 40 MeV/c • Momentum Spread : ���������������� �������� • phase rotation • ±3% (from ±30%) ��������������� ���������������� • Beam Repetition • 100 - 1000 Hz �������� • due to repetition of kicker ����������� ��������� magnets of the muon �������� ��������������� ��������� ������ storage ring. • Beam Energy Selection ���

  17. ... To Make Narrow Beam Energy Spread • A technique of phase rotation • Proton beam pulse should be is adopted. narrow (< 10 nsec). • The phase rotation is to • Phase rotation is a well- decelerate fast beam particles established technique, but and accelerate slow beam how to apply a tertiary beam particles. like muons (broad emittance) ? • To identify energy of beam particles, a time of flight (TOF) from the proton bunch is used. • Fast particle comes earlier and slow particle comes late.

  18. Phase Rotation for a Muon Beam Use a muon storage ring ? (1) Use a muon Storage Ring : A muon storage ring would be better and realistic than a linac option because of reduction of # of cavities and rf power. (2) Rejection of pions in a beam : At the same time, pions in a beam would decay out owing to long flight length. Which type of a storage ring ? (1) cannot be cyclotron, because of no synchrotron oscillation. (2) cannot be synchrotron, because of small acceptance and slow acceleration. Fixed field Alternating Gradient Ring (FFAG)

  19. R&D on the PRISM-FFAG Muon Storage Ring at Osaka University PRISM-FFAG (6 sectors) in RCNP, Osaka demonstration of phase rotation has been done . Ready to demo. phase rotation

  20. PRIME Detector

  21. PRIME Detector PRIME detector

  22. Potential Background for μ -e Conversion • Background rejection is the most important in searches for rare decays. • Types of backgrounds for μ - +N → e - +N are, • muon decay in orbit originate from muons Intrinsic • radiative muon capture stopping in the muon backgrounds • muon capture with particle emission stopping target. • radiative pion capture • muon decay in flight caused by beam particles, • pion decay in flight Beam-related such as electrons, pions, • beam electrons backgrounds muons, and anti-protons • neutron induced in a beam • antiproton induced • cosmic-ray induced Other • room-background induced anything others backgrounds • pattern recognition error

  23. PRIME to reject muon-induced backgrounds • (1) Rejection of protons and neutrons from muon nuclear capture • each stopped muon produces about 2 neutrons, 0.1 protons, and two photons. In paricular, protons are problematic. • curved solenoid transport system to reject low energy charged particles and neutral particles • remove primary as well as secondary and tertiary..... • more than 360 degree curve might be needed....

  24. 上流カーブドソレノイドの補正磁場 Selection of Charge and Momentum in Curved Solenoids • A center of helical trajectory of • This drift can be compensated charged particles in a curved by an auxiliary field parallel to solenoidal field is drifted by the drift direction given by � � � � B comp = p 1 1 D = p 1 1 cos θ + qB θ bend cos θ + qr cos θ 2 cos θ 2 D : drift distance p : Momentum of the particle B : Solenoid field q : Charge of the particle ! bend : Bending angle of the solenoid channel r : Major radius of the solenoid p : Momentum of the particle ! : atan(P T /P L ) q : Charge of the particle ! : atan(P T /P L ) • This can be used for charge and momentum selection. Tilt angle=1.43 deg.

  25. EM Physics for Particle Trajectories in Toroidal Magnetic Field • For helical trajectory in a vertical shift curved mag. field, a centrifugal force gives E in the radial direction. • To compensate a vertical shift, an electric field in E the opposite direction shall be applied, or a vertical mag. field that produces the desired electric field by v x B, can be applied. B (perpendicular to screen)

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