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The PRISM project Akira SATO Osaka University Project X Physics Workshop at FNAL 9-10 November 2009

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Page 1: The PRISM project - indico.fnal.gov fileThe PRISM project Akira SATO Osaka University Project X Physics Workshop at FNAL 9-10 November 2009

The PRISM projectAkira SATOOsaka University

Project X Physics Workshop at FNAL9-10 November 2009

Page 2: The PRISM project - indico.fnal.gov fileThe PRISM project Akira SATO Osaka University Project X Physics Workshop at FNAL 9-10 November 2009

Outline• Limits for the COMET and Mu2e experiment

• signal sensitivity

• high-Z stopping material

• PRISM concept

• R&Ds

• PRISM Task Force

• Summary

Page 3: The PRISM project - indico.fnal.gov fileThe PRISM project Akira SATO Osaka University Project X Physics Workshop at FNAL 9-10 November 2009

Muon - Electron Conversion

1s state in a muonic atom Neutrino-less muonnuclear capture

(=μ-e conversion)

B(µN eN) = (µN eN)(µN N ' )

nucleus

µ

muon decay in orbit

nuclear muon capture

µ + (A, Z)µ + (A,Z 1)

µ e

µ + (A, Z) e + (A,Z )

signal : mµ ! Bµ " 105MeV

Page 4: The PRISM project - indico.fnal.gov fileThe PRISM project Akira SATO Osaka University Project X Physics Workshop at FNAL 9-10 November 2009

R. Coleman Fermilab NuFact09 3

Production

Solenoid

Transport

Solenoid

Detector

Solenoid

Proton

Target

Target

ShieldingMuon Beam

Collimators

Tracker

Calorimeter

Pions Electrons

Muons

Muon

Stopping Target

Mu2e Muon Beamline- follows MECO design more information at http://mu2e.fnal.gov

Muons are collected, transported, and

detected in solenoidal magnets

COMET and Mu2e(MECO-type): B(µ! + Al ! e! + Al) < 10!16

Solenoid channel Stop µ- at the stopping targets. ID single electron from the target and measure its energy precisely.

Suppress backgrounds strongly.StoppingTarget

ProductionTarget

The MECO type experiments have some limitation on achievable sensitivity and physics studies.

Page 5: The PRISM project - indico.fnal.gov fileThe PRISM project Akira SATO Osaka University Project X Physics Workshop at FNAL 9-10 November 2009

Decay-in-Orbit Background

• To distinguish the signals from the DIO backgrounds, electron energy must be reconstructed with sufficient resolution. The present resolution is dominated by the energy struggling in the stopping target.

BR~10-16

Page 6: The PRISM project - indico.fnal.gov fileThe PRISM project Akira SATO Osaka University Project X Physics Workshop at FNAL 9-10 November 2009

Decay-in-Orbit Background (cont.)

• To achieve a signal sensitivity < 10-18, we need improve the energy resolution.• Thinner stopping targets with a sufficient muon stopping efficiency is

necessary. --> Mono-energetic muon beam is useful!

BR~10-18

Page 7: The PRISM project - indico.fnal.gov fileThe PRISM project Akira SATO Osaka University Project X Physics Workshop at FNAL 9-10 November 2009

Target dependence of µ-e conversion

• Once a signal of the µ-e conversion is observed, one can obtain information on models of the new physics, by changing the target material, even if µ→eγ is not observed.

• Contribution of different type of LFV operators is different from each nuclei.• Maximal in the intermediate

nuclei• Significantly Different Z

dependence for heavy nuclei• BUT, higher Z target makes

shorter µ lifetime in a muonic atom.

• Al : 880ns, Ti:329ns, Pb : 82ns

C. Target dependence of ! ! e conversion

In principle, any single-operator model can be testedwith two conversion rates, even if! ! e" is not observed.To illustrate this point, we update the analysis of Ref. [6]and plot in Fig. 3 the conversion rate (normalized to therate in aluminum) as a function of the Z of the targetnucleus, for the four classes of single-operator modelsdefined above. Compared to Ref. [6], the novelty here isthe inclusion of a second vector model (V!Z").

The results of Fig. 3 show some noteworthy features.First, we note the quite different target dependence of theconversion rate in the two vector models considered. Thiscan be understood as follows: In the case of the V!"" model,the behavior in Fig. 3 simply traces the Z dependence of

V!p" (the photon only couples to the protons in the nu-cleus). On the other hand, in the case of the V!Z" model, theZ boson couples predominantly to the neutrons in the

nucleus and the target dependence of the ratio V!n"=V!p" #!A$ Z"=Z generates the behavior observed in Fig. 3.Next, let us focus on the actual discriminating power of

the Z dependence. Clearly, the plot shows that the modeldiscriminating power tends to increase with Z. This is asimple reflection of the fact that the whole effect is ofrelativistic origin and increases in heavy nuclei. So in anideal world, in order to maximize the chance to discrimi-nate among underlying models, one would like to measurethe conversion rate in a light nucleus, say aluminum ortitanium, as well as in a large-Z nucleus, like lead or gold.This simplified view, however, has to be confronted bothwith theoretical uncertainties and the actual experimentalfeasibility. Concerning the uncertainties, a simple analysisshows that the dominant uncertainty coming from thescalar matrix elements almost entirely cancels when takingratios of conversion rates (even using the conservativerange y2 %0;0:4& for the strange scalar density matrixelement). Moreover, in the large-Z tail of the plot, someresidual uncertainty arises from the input on the neutrondensity profile. When polarized proton scattering data ex-ists, the uncertainty on the ratios of conversion rates be-comes negligible. This point is illustrated by Table I, wherewe report the detailed breakdown of uncertainties in theratios B!!e!Ti"=B!!e!Al" and B!!e!Pb"=B!!e!Al". Forother targets, the uncertainty induced by neutron densitiesnever exceeds 5% [6]. The conclusions of this exercise arethat(i) The theoretical uncertainties (scalar matrix elements

and neutron densities) largely cancel when we take aratio.

(ii) As evident from Fig. 3, a realistic discriminationamong models requires a measure of B!!e!Ti"=B!!e!Al" at the level of 5% or better, or alternatively

20 40 60 800

1

2

3

4

Z

Be;

ZB

e;A

l

V(Z)

V(!)

S

D

FIG. 3 (color online). Target dependence of the ! ! e con-version rate in different single-operator dominance models. Weplot the conversion rates normalized to the rate in aluminum(Z ' 13) versus the atomic number Z for the four theoreticalmodels described in the text: D (blue), S (red), V!"" (magenta),V!Z" (green). The vertical lines correspond to Z ' 13!Al", Z '22!Ti", and Z ' 83!Pb".

TABLE I. Ratios of conversion rates in titanium and lead overaluminum, in each of the four single-operator models: scalar (S),dipole (D), vector 1 (photon coupling to the quarks), and vector 2(Z boson coupling to the quarks). In the scalar model, the scalarform factor induces a negligible uncertainty in the ratios involv-ing two targets (denoted by the subscript y). In the case of leadover aluminum, the small uncertainty is dominated by theneutron density input (denoted by the subscript #n).

S D V!"" V!Z"

B!!!e;Ti"B!!!e;Al" 1:70( 0:005y 1.55 1.65 2.0

B!!!e;Pb"B!!!e;Al" 0:69( 0:02#n

1.04 1.41 2:67( 0:06#n

20 40 60 800.000

0.001

0.002

0.003

0.004

0.005

0.006

0.007

Z

Be;

ZB

e

FIG. 2 (color online). Ratio R!Z" of ! ! e conversion overB!! ! e"" versus Z in the case of the dipole-dominance model.

CIRIGLIANO, KITANO, OKADA, AND TUZON PHYSICAL REVIEW D 80, 013002 (2009)

013002-6

V.Cirigliano et al, Phys. Rev. D 80 013002 (2009)

Z-like vector

Photon-like vector

Photonic dipole

Higgs-like scalar

Al Ti Pb

Page 8: The PRISM project - indico.fnal.gov fileThe PRISM project Akira SATO Osaka University Project X Physics Workshop at FNAL 9-10 November 2009

Time distribution of backgrounds and signal• The muons stopped in the muon-

stopping target have the lifetime of a muonic atom. The time distribution of muon decays with the distribution of muon arrival timing is shown in Figure.

• Huge prompt BG exists just after the prompt timing. BUT Some beam-related backgrounds would come even after the prompt timing. Therefore, the measurement time window is selected to start after the prompt timing.

• The time window acceptance depends on the muon lifetime.

Arb

itrar

y U

nit

10

Prompt Background

Stopped Muon Decay

Main Proton Pulse10 p/pulse

8

(µs)Time

100 ns

1.1 µs

Arb

itrar

y U

nit

10

Prompt Background

Stopped Muon Decay

Main Proton Pulse10 p/pulse

8

Timing Window

(µs)Time

Signal

100 ns

1.1 µs

0 T1 Tp

Al

high-Z

Page 9: The PRISM project - indico.fnal.gov fileThe PRISM project Akira SATO Osaka University Project X Physics Workshop at FNAL 9-10 November 2009

Timing window selection efficiencies for COMET

Proton Pulse Interval (ns)0 500 1000 1500 2000 2500 3000

Effic

ienc

y

0

0.1

0.2

0.3

0.4

0.5

0.6

0.7Timing Window Cut Efficiency: Gold, t1=700ns, PPW=100ns

h6Entries 532100Mean 277.3RMS 132.9Underflow 0Overflow 0Integral 2.554e+04

Time (ns)0 1000 2000 3000 4000 5000 6000 7000 8000

Num

ber o

f Eve

nts (

a.u.

)

0

200

400

600

800

1000

h6Entries 532100Mean 277.3RMS 132.9Underflow 0Overflow 0Integral 2.554e+04

Decay Time: Gold, PPW=100ns-µh6

Entries 532100Mean 1054RMS 866.7Underflow 0Overflow 3.462Integral 2.554e+04

Time (ns)0 1000 2000 3000 4000 5000 6000 7000 8000

Num

ber o

f Eve

nts (

a.u.

)

020406080

100120140160180200220240

h6Entries 532100Mean 1054RMS 866.7Underflow 0Overflow 3.462Integral 2.554e+04

Decay Time: Aluminum, PPW=100ns-µ

Proton Pulse Interval (ns)0 500 1000 1500 2000 2500 3000

Effic

ienc

y

0

0.1

0.2

0.3

0.4

0.5

0.6

0.7Timing Window Cut Efficiency: Aluminum, t1=700ns, PPW=100ns

Proton Pulse Interval (ns)0 500 1000 1500 2000 2500 3000

Effic

ienc

y

0

0.1

0.2

0.3

0.4

0.5

0.6

0.7Timing Window Cut Efficiency: Titanium, t1=700ns, PPW=100ns

h6Entries 532100Mean 519.7RMS 345.3Underflow 0Overflow 0Integral 2.554e+04

Time (ns)0 1000 2000 3000 4000 5000 6000 7000 8000

Num

ber o

f Eve

nts (

a.u.

)0

100

200

300

400

500h6

Entries 532100Mean 519.7RMS 345.3Underflow 0Overflow 0Integral 2.554e+04

Decay Time: Titanium, PPW=100ns-µ

effi. = 0.37 effi. = 0.20 effi. = 0.01

Al (τ=864ns) Ti (τ=330ns) Au (τ=88ns)t1=700ns, Tp=1314ns

To measure BR with a high-Z target, the beam related backgrounds (pion radiative decay, beam flash etc) must be highly suppressed.

Page 10: The PRISM project - indico.fnal.gov fileThe PRISM project Akira SATO Osaka University Project X Physics Workshop at FNAL 9-10 November 2009

Summary of limits for the MECO type experiments• A signal sensitivity < 10-17 would be impossible with the MECO-type

experiments.• large flux of prompt backgrounds. ex. pion radiative decay etc• thick stopping target makes insufficient electron energy

resolution. • Measurement efficiency with high-Z stopping target would be poor.

Page 11: The PRISM project - indico.fnal.gov fileThe PRISM project Akira SATO Osaka University Project X Physics Workshop at FNAL 9-10 November 2009

Summary of limits for the MECO type experiments• A signal sensitivity < 10-17 would be impossible with the MECO-type

experiments.• large flux of prompt backgrounds. ex. pion radiative decay etc• thick stopping target makes insufficient electron energy

resolution. • Measurement efficiency with high-Z stopping target would be poor.

A mono-energetic and pure muon beam can solve these issues.

The next generation µ-e conversion experiment with PRISM!

Page 12: The PRISM project - indico.fnal.gov fileThe PRISM project Akira SATO Osaka University Project X Physics Workshop at FNAL 9-10 November 2009

Further Background Rejection to < 10-18

Beam-related Background

Extinction at muon beam

Pionbackground

long muon beam-line

Cosmic-raybackground

low-duty running

muon storage ring

fast kickers

100 Hz rather than 1 MHz

Muon DIO &Beam flush

narrow muon beam spread

1/10 thickness muon stopping target

pure muon beam

mono-energetic muon beam

Page 13: The PRISM project - indico.fnal.gov fileThe PRISM project Akira SATO Osaka University Project X Physics Workshop at FNAL 9-10 November 2009

High intensityintensity : 1011-1012µ±/secbeam repetition :100-1000Hzkinetic energy : 20MeV(=68MeV/c)

Narrow energy spreadkinetic energy spread : ±0.5-1.0MeV

Less beam contaminationcontamination < 10-18

PRISM : Phase Rotated Intense Slow Muon source

PRIME : PRIsm Muon to Electron Conv. Experiment

sensitivity of µ→e ∼ 10-18

Page 14: The PRISM project - indico.fnal.gov fileThe PRISM project Akira SATO Osaka University Project X Physics Workshop at FNAL 9-10 November 2009

To Make Narrow Beam Energy Spread• A technique of phase rotation is

adopted.

• The phase rotation is to decelerate fast beam particles and accelerate slow beam particles.

• 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.

• Proton beam pulse should be narrow (< 10 nsec).

• Phase rotation is a well-established technique, but how to apply a tertiary beam like muons (broad emittance) ?

NuFact03@Colombia University2003/6/6

Phase RotationPhase Rotationmethod to achieve a beam of narrow energy spreadmethod to achieve a beam of narrow energy spread

! Phase Rotation = decelerateparticles with high energy andaccelerate particle with lowenergy by high-field RF

! A narrow pulse structure (<1 nsec)of proton beam is needed toensure that high-energy particlescome early and low-energy onecome late.

Page 15: The PRISM project - indico.fnal.gov fileThe PRISM project Akira SATO Osaka University Project X Physics Workshop at FNAL 9-10 November 2009

Japanese staging plan of mu-e conversion

StoppingTarget

ProductionTarget

B(µ! + Al ! e! + Al) < 10!16

1st Stage : COMET

•without a muon storage ring.•with a slowly-extracted pulsed proton beam.•doable at the J-PARC NP Hall.•regarded as the first phase / MECO type•Early realization

2nd Stage : PRISM/PRIME

•with a muon storage ring.•with a fast-extracted pulsed proton beam.•need a new beamline and experimental hall.•regarded as the second phase.•Ultimate search

B(µ! + Ti ! e! + Ti) < 10!18

Page 16: The PRISM project - indico.fnal.gov fileThe PRISM project Akira SATO Osaka University Project X Physics Workshop at FNAL 9-10 November 2009

5 m

Capture Solenoid

Matching Section

Solenoid

RF Power Supply

RF AMP

RF Cavity

C-shaped

FFAG Magnet

Ejection System Injection System

FFAG ringDetector

PRISM : Super-muon sourcePRIME : µ-N→e-N Search with PRISM

Developed2003-2009

• Intensity : 1011-1012µ±/sec, 100-1000Hz• Energy:20±0.5 MeV (=68 MeV/c)• Purity:π contamination < 10-20

Page 17: The PRISM project - indico.fnal.gov fileThe PRISM project Akira SATO Osaka University Project X Physics Workshop at FNAL 9-10 November 2009

PRISM-FFAG

• Functions• makes monoenergetic muons:phase rotation• reduces π in the beam:long flight length

• Requirements & R&D items• Large acceptance FFAG-ring

• Horizontal:38000 π mm mrad

• Vertical :5700 π mm mrad

• Momentum: 68MeV/c +- 20%

• High field grad. RF system (170kV/m = 2MV/turn)• Quick phase rotation

• ~1.5µs

Page 18: The PRISM project - indico.fnal.gov fileThe PRISM project Akira SATO Osaka University Project X Physics Workshop at FNAL 9-10 November 2009

6-sector PRISM-FFAG at RCNP, Osaka Univ.

Page 19: The PRISM project - indico.fnal.gov fileThe PRISM project Akira SATO Osaka University Project X Physics Workshop at FNAL 9-10 November 2009

PRISM Task Force• The PRISM-FFAG Task Force was proposed and discussed

during the last PRISM-FFAG workshop at IC (1-2 July’09).

• The aim of the PRISM-FFAG Task Force is to address the technological challenges in realizing an FFAG based muon-to-electron conversion experiment, but also to strengthen the R&D for muon accelerators in the context of the Neutrino Factory and future muon physics experiments.

• It was proposed to achieve a conceptual design of the PRISM machine at the end of 2010/beginning 2011.

Page 20: The PRISM project - indico.fnal.gov fileThe PRISM project Akira SATO Osaka University Project X Physics Workshop at FNAL 9-10 November 2009

PRISM Task Force (cont.)• The following key areas of activity were identified and proposed to

be covered within the Task Force:• - the physics of muon to electron conversion,

- proton source,- pion capture,- muon beam transport,- injection and extraction for PRISM-FFAG ring,- FFAG ring design including the search for a new improved version,- FFAG hardware R&D for RF system and injection/extraction kicker and septum magnets.

• Please join! [email protected]

Page 21: The PRISM project - indico.fnal.gov fileThe PRISM project Akira SATO Osaka University Project X Physics Workshop at FNAL 9-10 November 2009

Summary• COMET and Mu2e has the limitation on the achievable sensitivity

(can not go < 10-17) and usage of high-Z material as a stopping target to study the nature of the new physics.

• To solve these issues, we need to modify and/or add some devices to the MECO type setup. PRISM/PRIME is a solution using a muon storage ring. LOI submitted to J-PARC. But needs more R&Ds.

• Project X could be nice proton driver for PRISM/PRIME type experiments to get BR<10-18. Needs studies and discussions.

• The PRISM-Task Force was established to make realistic design of a PRISM based µ-e conversion experiment as an ultimate experiment. Your collaboration is welcomed!