Progress & Challenges

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MICE collaboration meeting 12 at Frascati

-- Introduction --

MICE: progress and challenges

MICE collaboration meeting Alain Blondel 26-29 June 2005 1

Why MICE?

Based on Muon collider ideas and development (Palmer et al, 92->), the Neutrino Factory concept (Geer, 1998) resonated in 1998 with the final demonstration of Atmospheric Neutrino Oscillations by the SuperK Collaboration.

International workshops:

NUFACT 99 (Lyon, France)

NUFACT 00 (Montery, California)

NUFACT 01 (Tsukuba, Japan)

NUFACT 02 (London, UK)

NUFACT 03 (Columbia,NY,USA)

NUFACT 04 (Osaka, Japan)

NUFACT 05 (Frascati,Italy)

 Neutrino Factory is the ultimate tool for study of Neutrino Oscillations

-- unique source of high energy n

--reach/sensitivity better by order(s) of magnitude wrt other techniques (e.g. super-beams) for e m +  e + n e

_ n m

* q

1 3

*

** matter effects **

*** leptonic CP violation ***

****

n e

 n m

and

n t

****

NB : leptonic CP violation is a key ingredient in the leading explanations for the mystery of the baryon-antibaryon asymmetry in our universe

MICE collaboration meeting Alain Blondel 26-29 June 2005 2

MICE collaboration meeting Alain Blondel 26-29 June 2005

~NOvA +PD

3

encouraging signs from CERN… report from Scientific Policy Committee to council

Recommendations

• CERN should make every reasonable effort to deliver the approved p.o.t. to CNGS.

• Future neutrino facilities offer great promise for fundamental discoveries. CERN should join the world effort in developing technologies for new facilities : Beta beams, Neutrino Factory …wherever they are sited.

• Focus now on enabling CERN to do the best choice by

2010 on future physics programme.

• Explore further synergies with EURISOL

17 December 2004 Council Meeting, J.Feltesse

13

MICE collaboration meeting Alain Blondel 26-29 June 2005 4

An ambitious neutrino programme is a distinct possibility, but it must be well prepared to have a good proposal in time for the big decision period in 2010 (Funding window: 2011-2020)

Avenues identified as promising a) Superbeam alone + large detector(s) (e.g. T2HK, NOvA) a) SuperBeam + Beta-Beam + Megaton detector (SB+BB+MD) Fréjus b) Neutrino Factory (NuFact) + magnetic detector (40kton)+…

The physics abilities of the neutrino factory are superior but….. « what is the realistic time scale? »

(Hardware) cost estimate of a neutrino factory ~1B€ + detectors.

This needs to be verifed and ascertained on a localized scenario (CERN,

RAL…) and accounting.

The cost of a (BB+SB+MD) is not very different

Cost

/ physics performance / feasibility comparison needed

‘scoping study’

MICE collaboration meeting Alain Blondel 26-29 June 2005 5

Physics compare performance of various options on equal footing of parameters and conventions and agreed standards of resolutions, simulation etc.

identify tools needed to do so

(e.g. Globes upgraded) propose « best values » of baselines, beam energies etc..

MICE and the SCOPING STUDY…

Detectors (NEW!)

Water Cherenkov (1000kton)

Magnetized Iron Calorimeter (50kton)

Low Z scintillator (100 kton)

Liquid Argon TPC (100 kton)

Hybrid Emulsion (4 kton)

Peter Dornan

Near detectors (and instrumentation)

AB

Accelerator: M.Zisman

-- proton driver (energy, time structure and consequences)

-- target and capture (chose target and capture system)

-- phase rotation and cooling

-- acceleration and storage + Ken Long evaluate economic interplays and risks include a measure of costing and safety assessment

MICE collaboration meeting Alain Blondel 26-29 June 2005 6

Time scales:

NUFACT05 (Sunday 26 June 2005) launch of scoping study

September 2005: ISS report0

NUFACT06 (summer 2006) discussion of results of scoping study

September 2006 ISS report

2007 full design study proposal

2010 conclusions of Design Study & CDR

NB: This matches well the time scales set up at CERN

MICE collaboration meeting Alain Blondel 26-29 June 2005 7

Particle physicist:

Q: Can a Neutrino Factory be built?

Accelerator physisicst:

A: YES!

(US Study II, CERN) but… it is expensive, and many ingredients have never been demonstrated!

 R&D is needed. (est. 5yrs) to

1. ascertain performance

2. reduce costs among critical items:

***Target***

*** Acceleration ***

*** COOLING ***

Cooling component development programme+ ‘blast test’:

8

principle:

IONIZATION COOLING

reality (simplified)

this will surely work..!

….maybe…

A delicate technology and integration problem

Need to build a realistic prototype and verify that it works (i.e. cools a beam)

Difficulties lay in particular in

 operating RF cavities in Mag. Field,

 interface with SC magnets and LH2 absorbers

What performance can one get?

Difficulty: affordable prototype of cooling section only cools beam by 10%, while standard emittance measurements barely achieve this precision.

Solution: measure the beam particle-by-particle state-of-the-art particle physics instrumentation will test state-of-the-art accelerator technology.

MICE collaboration meeting Alain Blondel 26-29 June 2005

 RF Noise!!

9

10% cooling of 200 MeV/c muons requires ~ 20 MV of RF single particle measurements => measurement precision can be as good as

D ( e out never done before either…

/

e in

) = 10

-3

Spectrometer solenoid 1

Matching coils 1&2

Focus coils 1

Coupling Coils 1&2

Focus coils 2 Focus coils 3

Matching coils 1&2

Spectrometer solenoid 2 m

Beam PID

TOF 0

Cherenkov

TOF 1

RF cavities 1 RF cavities 2

Variable

Diffuser

Liquid Hydrogen absorbers 1,2,3

Incoming muon beam

Trackers 1 & 2 measurement of emittance in and out

MICE collaboration meeting Alain Blondel 26-29 June 2005

Downstream particle ID:

TOF 2

Cherenkov

Calorimeter

10

Muon Ionization Cooling Experiment

Aims: demonstrate feasibility and performance of a section of cooling channel

Main challenges:

RF in magnetic field!

10 -3 meas. of emittance

Safety issues

4T spectrometer II

Final PID:

TOF

Cherenkov

Calorimeter

Cooling cell (~10%) b =5-45cm, liquid H

2

, RF

Status:

Approved at RAL(UK)

First beam: 04-2007

Funded in: UK,CH,JP,NL,US

Requests: Be,CH,It,JP,US

4T spectrometer I

TOF

Singlem beam

~200 MeV/c

Some prototyping:

Liquid-hydrogen absorbers

200MHz RF cavity with beryllium windows

11

Some challenges of MICE:

1. Operate RF cavities of relatively low frequency (200 MHz) at high gradient

(16 MV/m) in highly inhomogeneous magnetic fields (1-3 T) dark currents (can heat up LH

2

), breakdowns

2. Hydrogen safety (substantial amounts of LH

2 in vicinity of RF cavities)

3. Emittance measurement to relative precision of 10 -3 in environment of RF bkg requires low mass and precise tracker low multiple scattering redundancy to fight dark current induced background excellent immunity to RF noise require complete set of PID detectors (INFN)

And…

4. Obtaining funding for R&D towards a facility that is not (yet) in the plans of a major lab

MICE collaboration meeting Alain Blondel 26-29 June 2005 12

NUFACT00

2000-2001

MICE is an international effort from the start.

NUFACT01 7:30 am

Sept. 2001

November 2001

January 2002

June 2002

January 2003

July 2003

October 2003

December 2003

June 2004

20 December 2004

Re-activated the recognized need for muon cooling expt

Workshops on Muon Cooling Experiment

(CERN, Chicago, London)

Steering group formed

Workshop at CERN where final experiment took shape.

Letter of Intent (LOI) submitted to PSI and RAL

PSI cannot host experiment, will collaborate (beam solenoid)

RAL IPRP Review Panel encouraged submission of a proposal

Proposal submitted

Recommendation by International Peer Review Panel

‘Scientific approval’ letter by RAL CEO JohnWood

Project Manager appointed (P. Drumm, RAL)

RAL CM: collaboration charter approved

Gateway 1 review

Gateway 1 passed on ‘amber’

Gateway 2/3 passed 10 green + 4 amber (MICE PHASE I)

March 2005 Release of funding approved by PPARC and CCLRC 9.7 M£

MICE collaboration meeting Alain Blondel 26-29 June 2005 13

at this point MICE (PhaseI) is an approved and funded project in 5 countries

-- UK: 9.7M£

-- USA: 1.2 M$ approved for next three years (NSF+DOE)

( +RF source + MRI proposal -- some success)

+ propose to build solenoid magnet within MC budget

(+ longer term plan for Coupling coil) (Zisman at CB)

-- Japan: US-Japan ~$100k/yr , UK-Japan (travel funds)

(+ 500k$ requested)

-- Switzerland: PSI solenoid + Uni-Geneva-NSwissF (80KCHF/yr)+ 1 PDA+1PhDS

-- Netherlands: Mag probes (in production!) + 1 PhDS

+ Proposal submitted in Italy (TOF, Calorimeter) and Belgium (Cherenkov)

MICE is CERN recognized experiment RE11.

MICE collaboration meeting Alain Blondel 26-29 June 2005 14

m

-

PHASE I

implementation in steps

STEP I:

April 2007 physics-based: understanding of systematics

STEP II:

October 2007 all configurations successfully matched optically

STEP III:

2008

PHASE II

STEP IV:

2008

MICE collaboration meeting Alain Blondel 26-29 June 2005

STEP V

2008?

STEP VI

2009?

15

MICE is being designed simulated reviewed

MOU’ed dug prototyped and built!

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SIMULATION

-- beam line : Turtle (Kevin Tilley) + G4beamline (Tom Roberts) match input beam (quads and dipoles) to MICE (solenoid)

600 ‘good muons’ per ISIS spill should be achievable

 10 -3 emittance measurement in 1 hr (stat)

(work to do for diffuser, variety of optics, etc…)

-- optics (Bob Plamer, Ulisse Bravar) ICOOL all steps of MICE have been optically matched

(but not to the beam) both in flip mode and solenoid mode

(proposed by Migliorati et al)

-- physics simulation (G4MICE, Y. Torun et al)

MICE collaboration meeting Alain Blondel 26-29 June 2005 17

SIMULATION and software.

‘Simple things should be easy and complicated things should be possible’

Sci-fi simulation of the measurement includes noise dead channels etc..

(Malcolm Ellis et al)

‘Students are taking over the project’

Yagmur Torun

G4MICE-ICOOL comparison Chris Rogers

Right ICOOL less than 10 -3 difference between true and reconstructed

E

Left G4MICE good to 20 ps and a few 100 keV

RF emission of X-rays (Rikard Sandstrom)

MICE collaboration meeting Alain Blondel 26-29 June 2005 18

requirements on spectrometer system:

1a reject incoming e, p, p ( TOF 0, TOF1)

1.b reject outgoing e => TOF2, Cerenkov + Calorimeter

2. measure x,y,Px, Py E (tracker) and t (TOF counters) to build 6D emittance particle by particle

3. resolution better than 10% of width at equilibrium emittance s 2 meas

= s 2 true

+ s 2 res

= s 2 true

[ 1+ ( s res

/ s true

)2 ]

(  correction less than 1%)

4. robust against noise from RF cavities

 Sci-Fi tracker was validated with calculations based on G4MICE

-- experimental input from prototype (dead channels, efficiency, resolution)

-- calculated spectrum and time structure of RF field emission based on LabG 800MHz

-- still will need to be scrupulous about multiple scattering in tracker  stepIII

Sci-fi prototype II presently assembled

 test at KEK in magnetic field (october)

MICE collaboration meeting Alain Blondel 26-29 June 2005 19

MICE collaboration meeting Alain Blondel 26-29 June 2005 20

Now same exercize needs to be done for TOF requires measured 50ps resolution

 double layer scintillator construction of TOF0 prototype this year

(Milano,Pavia, Padova, Geneva) funding available (GVA), proposal submitted (Italy)

50ps from tracker energy resolution

1%

TOF0 (R4998 Hamamatsu with Bicron scintillator)

MICE collaboration meeting Alain Blondel 26-29 June 2005 21

DAQ, controls and monitoring working group aims understand what instrumentation is needed and what data are needed at which frequency (per spill, per muon, independently) in order to perform comparison of data with simulation at the level of 10 -3 started to meet here at Frascati, will have dedicated workshop

(so far: Bross+Yoshida+Graulich+Radicioni+Drumm

 will need some accelerator physicists!)

MICE collaboration meeting Alain Blondel 26-29 June 2005 22

RF module

MICE is foresen with 8 RF cavities

Closed with curved Be windows

(increase gradient / MW RF power)

201 MHz

First cavity prototyped

(MUCOOL)

Completion in April 2005

RF power sources :

Will be assembled from equipement refurbished from Berkeley, Los Alamos, CERN, RAL.

Needed 8 MW peak power  23 MV acceleration

Operation at LN2 foreseen to increase Volts / MW

MICE collaboration meeting Alain Blondel 26-29 June 2005 23

RF circuits arrived from LBNL to Daresbury Lab.

Initial inspections of 4616 circuits

LBL equipment arrived Jan 05

Initial inspections

4616 circuits look ok !

MICE test area at Daresbury

Moss

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MICE Muon Beam

Design integration:

Beam line and shielding, cryogenics

MICE:

Support systems, RF, services, …

MICE collaboration meeting Alain Blondel 26-29 June 2005 25

MOU for PSI solenoid counter-signed

Paul Drumm

MICE Project Manager

Prof. John Wood RAL CEO

26

Hydrogen Safety

Safety Review process under way

Internal review organized in Berkeley in Dec. 2003

Reviewers:

D. Allspach (FNAL), G. Benincasa (CERN), M.

Seely (Jlab), L. Starritt (NASA), J. Weisend

(SLAC), J. Wells (RAL)

LH2

MLI

Evacuated buffer tank needed? NO

Burst valves and relief valves? YES

Separate vents for vacuum and hydrogen? YES

Detailed answers issued. Proceeding now to full safety revue (toward fall 2005) to be set up at this meeting

MICE collaboration meeting Alain Blondel 26-29 June 2005 27

Design and safety working group

nominated to ensure that

MICE is designed and built according to appropriate and safe engineering and according to RAL safety rules.

This will happen with 3 successive milestones internal audit external review (production readiness) external review (OK to operate)

RAL Review production reviews pertinent to PHASE I will have to be passed

***before end 2005***

…!

Review

Document

Review

RAL

Operate

FINAL

Document

Audit

MICE collaboration meeting Alain Blondel 26-29 June 2005 28

Time Line

If all goes well and funding is adequate, Muon Ionization cooling will have been demonstrated and measured precisely by

2009

At that time:

MINOS and CNGS will have started and measured D m

13

2

J-Parc-SK (and reactor expt?) will be about to start (

LHC will be starting as well q more precisely

13 measurement

)

It will be timely (…and not too soon!) to have by then a full design for a cost-optimized neutrino factory, with no questions about practical feasibility of ionization cooling

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MICE is getting REAL!

First beam 1st April 2007

**** 365*2 - 88 = 642 days to data taking !!!

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AIMS of the meeting:

• review ongoing activities

• design and safety reviews: where do we stand?

• are we on track to be ready to take data in April 2007?

• design of diffuser, impact on running strategy?

• see formation of DAQ Controls and Monitoring group

• continue to broaden simulation effort  analysis forum

• creation of editorial board foreseen in MICE constitution

NB: we had 6 contributions to PAC05

NB we strongly encourage everyone to document their work within the framework of MICE with MICE Notes!

MICE collaboration meeting Alain Blondel 26-29 June 2005 31

Editorial Board

This body approves publications from the Collaboration. Two types of publications are foreseen.

Collaboration Publications

These publications are issued as ‘MICE Collaboration’ publications and it is expected that all active members of the collaboration will sign. All analysis results from the experimental data are expected to be in this category as are descriptions of the experiment as a whole and its performance. These must be approved by the Editorial Board.

Limited Publications

Publications by a limited number of members of the collaboration concerning e.g. the construction and performance of specific subcomponents of the experiment. They are not issued as ‘MICE Collaboration’ publications, however it is recommended that these papers are also submitted to the Editorial Board for approval so that the management are aware of them and can advise of any possible conflicts with other members which may occur.

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