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Page 1: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar Villars 2004Villars 2004

Report on the SPSC Villars Meeting

September 22-28 2004

John DaintonUniversity of Liverpool, GB

(on behalf of the SPSC)

Page 2: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar Villars 2004Villars 2004

Report on the SPSC Villars Meeting

September 22-28 2004

John DaintonUniversity of Liverpool, GB

(on behalf of the SPSC)

1. Framework2. Machines and Beams3. Heavy Ions4. Neutrinos5. Soft and Hard Protons 6. Antiproton Physics7. Flavour Physics8. Other Topics9. Summary

Note 8/10/04: Overheads are here exactly as presented apart from a small number of bugs which have been fixed, and apart from the inclusion of some overheads skipped in the seminar because of time pressure.

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John DaintonVillars 2004

October 7th 2004CERN seminar

1. Framework1. Framework

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John DaintonVillars 2004

October 7th 2004CERN seminar ChargeCharge

“to review present and future activities and opportunities in fixed-target physics, and to consider possibilities and options for a future fixed target programme at CERN”

globally important

realistic (beams + resources)

short, intermediate, and long term

from the SPCSPSC not in approval/rejection mode !

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John DaintonVillars 2004

October 7th 2004CERN seminar

TimetableTimetable

“… groups working on fixed target experiments at CERN, and also groups which have in mind the submission of proposals for such experiments, to forward to the SPSC secretariat in due time a short report indicating their ideas and plans for the

future”

SPSC67 April 2004

11 submissions received +COMPASSDIRAC kπ atomsCNGS

committed beyond 2005}

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John DaintonVillars 2004

October 7th 2004CERN seminar

Submissions of InterestSubmissions of Interest

Expression of Interest to Measure Rare Kaon Decays at the CERN SPS (NA48-Future Working Group)A New Experimental Programme with Nuclei and Proton Beams at the CERN SPS (M. Gazdzicki for NA49 Colln) Electromagnetic processes in strong crystalline fields - exploring the Schwinger field (U.I. Uggerhoj for NA43 Colln)COMPASS 2005-201x (A. Magnon for NA58/COMPASS Colln)Atomic Spectroscopy and Collisions Using Slow Antiprotons(R.S. Hayano for AD-3/ASACUSA Colln)Hadron production measurements (J. Panman for PS214/HARP Colln)Possible Future Experimental Searches at CERN in Astroparticle Physics (K. Zioutas for the CAST Colln)Measurement of antimatter gravity with an (anti)matter wave interferometer (C. Regenfus, Physik Inst . Univ. Zürich)Expression of Interest: Study of dimuon and heavy-flavour production in proton-nucleus and heavy-ion collisionsAntihydrogen Laser Experiment Roadmap (J.S. Hangst)R&D for Antimatter Spectroscopy (Neutral Atom Trap (NEAT) Colln)

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John DaintonVillars 2004

October 7th 2004CERN seminar

Timetable contdTimetable contd

May 25-26: CERN SPL Workshop (also @ Villars)

June 5-8: High Intensity Workshop (INFN) HIF04 (also @ Villars)

SPSC68 July 6 2004

programme finalised (speakers fixed)

September 22 to 28: Villars

October: Seminar @ CERN

December: report to RB + SPC

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John DaintonVillars 2004

October 7th 2004CERN seminar

OrganisationOrganisation

topic chief convener conveners

anti-protons H Bialkowska

R Batley, M de Jong

G Hamel de Monchenault

neutrinos D Wark M Doser, M Piccolo

heavy flavorG Hamel de Monchenault

S ForteJ Ritman,A Schäfer

soft and hard hadrons

U StössleinM Doser, S Forte

S Kox

Heavy Ions L Kluberg I Brock, A Schäfer

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October 7th 2004CERN seminar

ProgrammeProgramme

Date Morning Afternoon

Wednesday Sept 22 CERN perspve+accelr MMWSPL

HIF Heavy Ion 1

Thursday Sept 23 Heavy Ion 2 Neutrino 1

Friday Sept 24 Neutrino 2Soft and hard hadron

physics 1

Saturday Sept 25Soft and hard hadron

physics 2 Anti-proton 1

Sunday Sept 26 Anti-proton 2 HF 1

Monday Sept 27 HF 2Other

Topics Discussio

n

Tuesday Sept 28Summary,

Discussion & Conclusions

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October 7th 2004CERN seminar

FormatFormat

Topic structure

Session 1 Session 2

1 keynote speaker(s) for status and outlook including and “beyond”CERN2 includes CERN experiment and CERN proto-experiment representatives and, if essential, also summariser(s) from other labs3 focussing on future strategy4 first draft of conclusions concerning physics directions

Keynoteintroduction1

Invited presentations

with discussion2

Further discussion3 Summary4

Invited speaker

experiments all convenors

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John DaintonVillars 2004

October 7th 2004CERN seminar

DocumentationDocumentation

Overheads

Submitted documents

WG Convenor summaries

Summary speaker’s conclusions

SPSC conclusions in Chair’s seminar overheads

Summary of conclusions and recommendations

written

SPSC members (= convenors + chair)

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October 7th 2004CERN seminar

2. Machines and Beams

2. Machines and Beams

Aymar, Benedikt,Cervelli, Elsener,Engelen, Garoby,

Gatignon, Palladino

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October 7th 2004CERN seminar

Users’ View of Future:pre Villars04

Users’ View of Future:pre Villars04

USERCERN

COMMITMENT*USERS’ WISHES

Short term(low cost)

Medium term(intermt cost~ asap !

Long term(high cost: >2013)

LHC Planned beamsUltimate

luminosityLuminosity upgrades

FT (COMPASS)7.2105 spills/y

?7.2105 spills/y

CNGS 4.51019 p/year Upgrade ~ 2

ISOLDE 1.92 A ** Upgrade ~ 5

Future beams > 2 GeV / 4 MW

EURISOL 1-2 GeV / 5 MW

* Reference value for analysis ** 1350 pulses/h – 3.21013 ppp

● as heard by HIP from users

Garoby

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John DaintonVillars 2004

October 7th 2004CERN seminar

UpgradesUpgrades

● beam loss irradiation @ high intensitymulti-turn ejection from PS (“island extractn”)

● period 0.6 s 0.9 s ?

> cost > worse PSB flexibility better

● intensity/SPS pulse increase CNGS flux- machine impedance (kickers, RF…) ?- injection energy ?- bunching in the PS ?

only

BenediktGaroby

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October 7th 2004CERN seminar

Without upgrades*Without upgrades*

2006 2007 2010 Basic user’s request

CNGS flux

[1019 pot/year]4.4* 4.2* 4.9* 4.5

FT spills[105 /year]

3.3 1.8 3.3 7.2

E Hall spills[106 /year]

1.3 2.3 2.3 2.3

NTOF flux[1019 pot/year]

1.4 1.6 1.6 1.5

ISOLDE flux [μA][no. pulses/hour]

1.841296

1.651160

1.741220

1.921350

72 bunch train for LHC at PS exit

[1011 ppb]1.5 1.5 1.5 1.3 (2**)

* w

ith

im

port

an

t ir

rad

n o

f P

S e

qu

ipt

** u

ltim

ate

beam

in

LH

C

BenediktGaroby

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October 7th 2004CERN seminar

With upgradesWith upgrades

Standard(i)

CNGS x2 batch(i)+(ii)

Linac 4(i)+(ii)+(iii)

Basic user’s

request

CNGS flux [1019 pot/year]

4.7 (4.5)

7.0 (4.5) 7.5 (4.5) 4.5

FT spills [105 /year]3.2

(3.4)3.0 (5.1) 3.2 (5.6) 7.2

E Hall spills [106/year]

2.3 2.3 2.3 2.3

NTOF flux [1019 pot/year]

1.7 1.6 1.7 1.5

ISOLDE flux [μA][no. pulses/hour]

3.02126

2.451722

6.22160

1.91350

72 bunch train for LHC at PS exit [1011 ppb]

1.5 1.5 2 1.3 (2*)

●(i) PSB repetition period of 0.9 s

(ii) 7x1013 ppp in SPS (iii) Linac4 injecting into PSB

BenediktGaroby

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John DaintonVillars 2004

October 7th 2004CERN seminar

Fixed target CNGSFixed target CNGS

FT vs. CNGS performance 2006, 2007, 2010

0

1

2

3

4

5

6

7

8

9

10

0 1 2 3 4 5 6 7 8CNGS protons on target [1019]

FT

sp

ills

[10

5]

2006

2007

2010

FT request 7.2E5 spills/year

CNGS request 4.5E19 protons/yearCNGS request

4.5 1019 pot/year

FT request7.2 105 spills/year

Without changes

Double batch + Linac4

Double batch

BenediktGaroby

●FT + CNGS share SPS cycles

●impossible to meet FT + CNGS demands

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John DaintonVillars 2004

October 7th 2004CERN seminar

Fixed target CNGSFixed target CNGS BenediktGaroby

●FT + CNGS share SPS cycles

FT + CNGS

LHC + CNGS

●impossible to get closer to FT + CNGS demands ?

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John DaintonVillars 2004

October 7th 2004CERN seminar

Scope of Future OptionsScope of Future Options BenediktGaroby

interest for

LHC upgradeNeutrino physics

beyond CNGS

Radio-active ion

beams (EURISOL

)

Others

Low energy50 Hz RCS

(~ 400 MeV/2.5 GeV)

ValuableVery interesting for super-beam

+ beta-beamNo ?

50 Hz SPL(~ 2 GeV )

ValuableVery interesting for super-beam

+ beta-beamIdeal

Spare fluxÞ

possibility to serve

more users

High energy8 Hz RCS

(30-50 GeV)Valuable

Very interesting for neutrino

factoryNo Valuable

New PS(30-50 GeV)

Valuable No No Valuable

1 TeV LHCinjector

Very interesting for luminosity

upgrade.Essential for

LHC energyx2

No No Valuable

synergy

Page 20: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

Strategy (and action)Strategy (and action) BenediktGaroby

● start 2004/5:- PS: multi-turn ejection- increase SPS intensity (impacts all machines)- 0.9s PSB repetition

● Linac 4 design construction decision @ end 2006

● prepare decision on optimum future accelerator - study of a Superconducting Proton Linac (SPL)- alternative scenarios for the LHC upgrade

context for SPSC strategy and input

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October 7th 2004CERN seminar

CERN 2004CERN 2004 Gatignon

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October 7th 2004CERN seminar

North 2004North 2004 Gatignon

CO

MPA

SS

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John DaintonVillars 2004

October 7th 2004CERN seminar

East 2004East 2004 Gatignon

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October 7th 2004CERN seminar

North: Heavy Ions >2005

North: Heavy Ions >2005

After the long shut-down ions will be injected into the SPS via LEIR.The LEIR project has been launched for filling the LHC with ions.Filling the SPS instead will require more resources.

If the ions are required for the SPS fixed target program and if therequired resources are made available, one might expect to get:

• Lead ions from 2009 (after PS-SPS-LHC ions running-in)• Other (lighter) ions depending on LHC ion physics program.

It should be noted that many relevant non-radioactive ion species are possible ‘in principle’, but with significant preparation time and effort.Note that North Area and LHC ions are exclusive if not the same ion

Possible intensities are up to 109 Pb54+ from LEIR per transfer (3.6 sec).They can be limited in LEIR with an interlock based on a BCT measurement.Limitation of flux in EHN1 requires new TAX blocks (up to 300 kCHF/beam).

It should be noted that ion injection via LEIR for fixed targethas not yet been studied in depth. More studies are requiredat the source, Linac3, LEIR, PS and at the SPS.

Gatignon

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October 7th 2004CERN seminar

North: µ & HadronsNorth: µ & Hadrons Gatignon

● M2 for COMPASS (approved)

- µ ≤ 190 GeV/c

- 2dary hadrons ≤ 280 GeV/c

- e ~ 40 GeV/c

● M2 for COMPASS (future?)

- primary p

- hyperons

● M2 intensity ?

rebuild CHF

radlim CHF

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John DaintonVillars 2004

October 7th 2004CERN seminar

North: Kaons > 2005North: Kaons > 2005

● to separate or not to separate ?- acceptance: unseparated ~ 100 x separated

- tag @ 109 Hz

+ K+ : 6.2% +: 71.1% p : 22.7%

- K- : 6.8% -: 90.8% p :2.4%

> x 40 K+ /year

Gatignon

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John DaintonVillars 2004

October 7th 2004CERN seminar

CERN LNGS = CNGS

CERN LNGS = CNGS

Elsener

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John DaintonVillars 2004

October 7th 2004CERN seminar

CERN LNGS = CNGS

CERN LNGS = CNGS

Elsener

● beam in 2006

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John DaintonVillars 2004

October 7th 2004CERN seminar

CNGS: making νCNGS: making ν Elsener

p + C (interactions) , K (decay in flight)

700 m 100 m 1000m 67 m

● largest intensity

● Eν for νe ντ

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October 7th 2004CERN seminar

CNGS HorizonCNGS Horizon

● nominal (1999)

- 2.4x1013 p /extraction

- 4.8x1013 p /cycle

- 4.5x1019 p /year

eg 200 days 55% efficiency LHC MD LHC fill FT

● 2nd look (2001)

- 3.5x1013 p /extraction

- 7x1013 p /cycle

- 13.8x1019 p /year

target rods ?windows ?heating: target, horn ?shielding ??

●R&D underwayNB decommissioning cost

>> construction cost

X3 ?

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John DaintonVillars 2004

October 7th 2004CERN seminar

ADAD Gatignon

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October 7th 2004CERN seminar

AD >2005AD >2005

● modified extraction

● degrader foils RFQD for ATRAP + ATHENA

● decelerator ring ELENA

5.3 MeV KEp 100 KeV ?-

● injection stacking intensity x 2 to 5

● PS beam 4 5 bunches intensity x 1.25

Gatignon

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John DaintonVillars 2004

October 7th 2004CERN seminar

Summary: FT beamsSummary: FT beams

● North Area @ SPS diverse beams

● East Hall @ PS DIRAC + … ?

● CNGS ≥ 2006; improving intensity ?

● ions ≥ ~ 2009

● CHF ? modernisation

● CHF ? new possibilities/opportunities

(test beams !)

context for SPSC strategy and inputun

para

lleled

varie

ty

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John DaintonVillars 2004

October 7th 2004CERN seminar

3. Heavy Ions3. Heavy Ions

Gadzicki, Haungs,Lourenco, Riunaud,

Satz

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John DaintonVillars 2004

October 7th 2004CERN seminar

SPbS PanoramaSPbS Panorama

The SP[b]S Panorama

photons

J/ψ

chemistrye+e-

HBT

spectra ● expt @ SPbS + theory QGP

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John DaintonVillars 2004

October 7th 2004CERN seminar

ChromodynamicPhase EquilibriaChromodynamicPhase Equilibria

● SPS @ phase transition

T

Early universeRHIC, LHC

B

Hadronicmatter

Critical endpoint

Quark-Gluon Plasma (QGP)

Nuclei

Chiral symmetrybroken

Chiral symmetryrestored

BaryonDominated HG

MesonDominated HG

Color superconductor

Neutron stars

QGP

SPS

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John DaintonVillars 2004

October 7th 2004CERN seminar

Critical PointCritical Point

● theoretical guidance model dependent

Stephanov

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John DaintonVillars 2004

October 7th 2004CERN seminar

target boxwindows

7 In targets

z-vertex (cm)

Indium beam

158 A GeV

Beam tracker station

vertex transverse coords determinedwith pixel telescope + beam tracker to

better than 20 mm accuracy

interaction z-vtx from rad hardpixel telescope ~ 200 µm accuracy

hadronic vertexdimuon vertex

(mass > 2 GeV)

Heavy Ions + NA60 PixelsHeavy Ions + NA60 Pixels NA60 - Lourenco

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John DaintonVillars 2004

October 7th 2004CERN seminar

Low mass dileptons Low mass dileptons

CERES/NA45

NA60400 GeV

σ

Mee Mµµ

● excess dileptons – thermal radiation ?

Page 40: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

SPSCSPSC

● immediate (SPSC) - NA60

p+In data open charm, ρ mass, thermal radn Pb+Pb highest energy density @ SPS

- NA49jet quenching @ RHIC

high pT quenching @ SPS ? complete Pb+Pb high pT hadron analysis

then pA referencethen high pT Cronin effect

data taking now

declared interest

declared interest

Page 41: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

SPSCSPSC

● longer term (SPSC) - chase and evaluate the critical point @ CERN

establish optimal theoretical signatures optimise experiments for signal and sensitivity

- unique @ CERN, timely even ≥ 2009, important

- ≥2009 CERN FT + LHC HI synergy

no overwhelming scientific needfor ion+ion FT < 2009

Page 42: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

4. Neutrinos4. Neutrinos

Blondel, Declais,Dydak, Gilardoni,

Haseroth, Lindroos,Mezzeto, Mosca

Nishikawa, Panman,Romanino, Rubbia

Page 43: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

71±571±5

Early Solar Neutrino Exps.

SNO

SuperK

Soudan II

MACRO

KamLAND

K2K

LSND

ν-oscillationsν-oscillations Wark

New KamLAND

Super-KL/E

Page 44: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

EigenstatesEigenstates

232

2210 mm uniquely defines the labelling

0221 m can have both

signs:by definition, 2

32m

Normal

11

22

33

normal

0232 m Normal

33

22

11

0232 m

inverted

e.g.:

(inverse hierarchical)

(degenerate)

321 mmm

321 mmm

e.g.:

(hierarchical)

(degenerate)

(neither)

321 mmm

321 mmm

321 m«mm

2ATM

232

2SUN

221

ΔΔ

ΔΔ

mm

mm

Romanino

Page 45: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

HierarchyHierarchy

~sin223

Solar + KamLAND

Super-K

Wark

● remarkable progress

Page 46: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

Next ?Next ?

● CNGS: OPERA ICARUS● better than hitherto (better than CKM?):

MINOS, KamLAND, Borexino?T2K νe appearancenearer, near, and far detectors

β–beam? CERNFrejus?

● θ13 pre-requisite for δ

● sign of Δm232 (or Δm13

2): crucial for Ών

● CP-violating phase δ

Page 47: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

Next ?Next ? Mezzetto

Page 48: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

OPERAOPERA

Pb

Emulsion layers

1 mm

Plastic base

• for the full detector:2 supermodules31 walls /

supermodule52 x 64 bricks /wall200 000 bricks

56 emulsion films / brick

~2 kTon (Pb) 0.04 kTon

emulsion

9 kt-yr

Δm2=1.2x10-3 eV2 2.7 eventsΔm2=2.4x10-3 eV2 11 eventsΔm2=5.4x10-3 eV2 54 events

● ready end 2006

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John DaintonVillars 2004

October 7th 2004CERN seminar

ICARUSICARUS

muon spectrometer≈2 kton Fe B=1.8 T

3m

●3 kt in LNGS 2005 ?

LAr drift

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John DaintonVillars 2004

October 7th 2004CERN seminar

ICARUSICARUS

2 64 1812

2

Wire coord. (m)

DriftCoord.

(m)

Zoom View3.9 m

1.3 m

Full 2D view from the Collection Wire Plane

T600 test: Run 308 - Evt 7

●”ultimate” vertex resolution: T600 ready … LNGS

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October 7th 2004CERN seminar

≡ T2K

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October 7th 2004CERN seminar

beam of < 1GeVKamioka

J-PARC(Tokai-village)

→ → xx disappearance

→ → ee appearanceNC measurement

0.75 MW 50 (40) GeV PS

Super-K: 50 ktonWater Cherenkov

~Mt “Hyper Kamiokande”

4MW 50GeV PS

CP violation proton decay

Approved exp (x102 of K2K)

Future Extension

“T2K” (Tokai-to-Kamioka)

“T2K” (Tokai-to-Kamioka)

LOI: hep-ex/0106019

Collaboration• Formed in May 2003• 12 countries, 52 institutions• 148 collaborators (w/o students)

Nishikawa

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October 7th 2004CERN seminar

StrategyStrategy

• High statistics by high intensity beam• Tune E at oscillation maximum• Sub-GeV beam

Low particle multiplicity suited for Water CherenkovGood E resolution : dominated by np

• Narrow band beam to reduce BG

0.75MW 50GeV-PS

Off-Axis beam Super-Kamiokande

Nishikawa

Page 54: Villars 2004

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October 7th 2004CERN seminar

T2K ScheduleT2K Schedule

• Possible upgrade in future4MW Super-J-PARC + Hyper-K ( 1Mt water

Cherenkov)CP violation in lepton sectorProton Decay

2004 2005 2006 2007 2008

SK full rebuild

T2K construction physics run K2K

2009

PS commisionning

Nishikawa

Page 55: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

Neutr

ino.

PPAP Mar. 25’04

…osc

illati

ons

Imperial College/RALDave Wark

Beta-beam study group

CERN: -beam baseline scenario

PS

Decay

Ring

Decay ring

Brho = 1500 Tm

B = 5 T

Lss = 2500 m

SPSISOL target & Ion source

SPL

Cyclotrons, linac or FFAG

ECR

Rapid cycling synchrotron

Nuclear Physics

MeV 86.1 Average

MeV 937.1 Average

189

1810

63

62

cms

cms

E

eFeNe

E

eLiHe

P. Zucchelli, Phys. Lett. B, 532 (2002) 166-172

Slide from M. Lindroos

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John DaintonVillars 2004

October 7th 2004CERN seminar

Neutr

ino.

PPAP Mar. 25’04

…osc

illati

ons

Imperial College/RALDave Wark

Beta-beam study group

CERN to FREJ USG

enev

e

Italy

130km

40kt400kt

CERN

SPL @ CERN2.2GeV, 50Hz, 2.3x1014p/pulse 4MWNow under R&D phase

Megatonne ?

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October 7th 2004CERN seminar

θ13 CP sensitivity

Towards NF HorizonTowards NF Horizon

● SPL superbeam ?

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October 7th 2004CERN seminar

SPL Proposed RoadmapSPL Proposed Roadmap

Consistent with the content of a talk by L. Maiani at the “Celebration of the Discovery of the W and Z bosons”. Contribution to a document to be submitted to the December Council (“CERN Future Projects and Associated R&D”).

Assumptions:• construction of Linac4 in 2007/10 (with complementary resources, before end of

LHC payment)• construction of SPL in 2008/15 (after end of LHC payments)

Task Name

LINAC4

Design ref inment

Construction

Commissioning

Start operation with PSB

SPL

Design ref inment

Construction

Linac4 displacement + commissioning

Start operation as PS Injector

12/31

12/30

2004 2005 2006 2007 2008 2009 2010 2011 2012 2013 2014 2015 2016

Linac 4 approval SPL

approvalLHC

upgradeR. Garoby

Warning: Compressor ring and detector (8 years) are not quoted Protons from the SPL ready in 2015

Gilardoni

Page 59: Villars 2004

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October 7th 2004CERN seminar

SPL SuperBeam FAQSPL SuperBeam FAQ

Q: Why 2.2 GeV for the proton driver?A: First design of the SPL which used the LEP cavities.

Q: What about increasing the proton energy ?A: Possible up to 3.5 GeV- 4 GeV with some caveats. Energy

optimization to tune the proton beam energy is in working stage (see next slides).

Q: Is the SPL SuperBeam strongly connected with the Frejus?A: Yes, due to low energy of proton beam no way to go further

than 130 km.

Q: What if instead of a Cherenkov detector one wants to use a Liquid Argon TPC ?

A: Possible if the experts are interested in the location (meaning not going to Japan)

Gilardoni

Page 60: Villars 2004

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October 7th 2004CERN seminar

SPL SuperBeam FAQSPL SuperBeam FAQ

Q: Why proposing the SPL Superbeam if JHF will have similar results?

A1: Unique synergy with the Beta Beam

A2: Learned from the Japanese style of working, and also from CERN style, every step carries the know-how for the next step. The next could be a NuFact.

A3: Different condition to repeat the same measurement. In particular different background.

Gilardoni

… but not first

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October 7th 2004CERN seminar

Proton Driver νProton Driver ν

● expensive

● likelihood improves

with synergy

● ν beam R&D for new technology

- target- cooling

(MICE)

● νe - β beam

νμ - superbeam

● ν Fact

Mezzetto

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October 7th 2004CERN seminar

SPSCSPSC

● ν physics has noble history at CERN

● ν physics is in a new golden era - CERN beginning again pivotal global role

● CNGS commitment to ~ end of decade vital - 2006 important: COMPASS then CNGS @ end 06 - CNGS crucial up to 2011 (window @ 4.5x1019pot/yr) - CNGS + COMPASS ? multi-turn xtraction

longer running period - no compelling case for extending CNGS beyond 2011 @ realisable pot/yr (< ~ 3x 4.5x1019pot/yr)

C2GT

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October 7th 2004CERN seminar

SPSCSPSC

● Future neutrino facilities offer great promise for fundamental discoveries (such as CP violation) in neutrino physics, and a post-LHC construction window may exist for a facility to be sited at CERN.

● CERN should arrange a budget and personnel to enhance its participation in further developing the physics case and the technologies necessary for the realization of such facilities. This would allow CERN to play a significant role in such projects wherever they are sited.

● A high-power proton driver is a main building block of future projects, and is therefore required.

● A direct superbeam from a 2.2 GeV SPL does not appear to be the most attractive option for a future CERN neutrino experiment as it does not produce a significant advance on T2K.

● We welcome the effort, partly funded by the EU, concerned with the conceptual design of a β-beam. At the same time CERN should support the European neutrino factory initiative in its conceptual design.

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October 7th 2004CERN seminar

SPSCSPSC

● Detectors – new detector technologies are necessary to take full advantage of the physics capabilities of future neutrino facilities. Examples of needed advances are cheaper, higher efficiency, large-area, light sensors and magnetized detectors capable of distinguishing electrons from positrons. Given its central role as Europe’s particle physics laboratory, CERN should support, participate, and coordinate such technical developments.

● Further hadron production experiments specifically designed to meet the needs of neutrino experiments are essential. There are several existing CERN detectors which could, with some modifications, fulfill this requirement. This would be a scientifically important and cost-effective use of CERN resources.

Page 65: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

5. Soft and Hard Protons5. Soft and Hard Protons

D’Hose, DiehlGasser, GninenkoMagnon, Malvezzi

Nemenov, PaulPolyakov, Seymour

Vestzergombi,

pivotal role of CERNThe stuff of Nobel Prizes !

Page 66: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

Hadron PhysicsHadron Physics

H1 ZEUS - DESY

GSI

● energy frontier colliders

● precision frontier colliders + FT

● intensity frontier

● theoretical symbiosis- lattice- ChPT

- pQCD BABAR - SLAC

CDF D0 - FNAL

Page 67: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

COMPASSCOMPASS

● 1996: proposal 1997: conditional approval 1999 – 2000: construction and installation 2001: commissioning run 2002 -2004: data taking µp and µp

● precision hadron structure- nucleon spin structure (valence sea)

● precision hadron dynamics - pQCD n-pQCD (Q2 pT

2) - resonant phenomena

● into the future: GPDs and precision st. functions

gluons

ap

pro

ved

Page 68: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

COMPASS ΔG/GCOMPASS ΔG/G

●finding charm

c

cσ(ΔG/G) proposal = 0.142002+3+4

σ(ΔG/G) = 0.24

-

h

hLeading process

h

hGluon radiation (Compton)

h

h

Photon Gluon Fusion (PGF)

●ΔG/G from high pT hadrons pairs

Page 69: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

COMPASS Hadron (≥2004)

COMPASS Hadron (≥2004)

●PT: Primakoff

●resonance -diffractive - Primakoff - central: glue enriched (WA102 …) - D* Ds* (FOCUS, BABAR, Belle, CLEO, SELEX)

- Λc* … - Ξcc localised (cc) excitation against light u/d

fast

slow

●270 GeV p + vertex detector

●150 days/year 2006-2010

Page 70: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

COMPASS beyond …COMPASS beyond …

●DIS: forward * Compton

- ∫pdf(x,t)●dt

●DVCS: * Compton- pdf(x,t)- p tomography ? partons across p

unpolarisedpolarised

d-d

Diehl

-

relevant at the time?

Page 71: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

DIRACDIRAC

“atomic pairs”

“free pairs”

●ππ and Kπ “atoms” - scattering lengths - PT

● data 2001 – 2003 (PS)

● setting up 2006 (PS)

● running 2007/8 (PS)

● planning > 2008 (SPS ?)

● excess at very small

pL and pT

● experimental = theoretical uncertainty @ SPS

≠ Ke decay

Page 72: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

SPSCSPSC

● FT hadron program remains very competitive

● COMPASS complete in medium term- ΔG/G- transversity, polarisability, spectroscopy- SPSC p.o.t. concern prioritise

● COMPASS longer term- GPD measurements would be unique

● DIRAC physics important SPS (accuracy)

● hadron resonances (pQ) in existing NA49 not compelling

Page 73: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

SPSCSPSC

● FT 2006: optimise running

- start early data for COMPASSoptimise data-taking efficiency

- run til CNGS ready

● FT > 2006 encourage multi-turn Xtraction

● FT >> 2006- intense ν @ CERN new lepton-hadron DIS

Page 74: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

6. Antiproton Physics6. Antiproton Physics

BeloshitzkyGabrielse, Hangst

Hayano, JungmannKostelecky, Quint

Regenfus, TesteraWidmann, Yamazaki

Page 75: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

Unique Physics at CERN

Unique Physics at CERN

● ASACUSA ATRAP ATHENA- “routine” production of H - antiprotonic He = p e -

● deceleration and capture of p

● production of H and He- yield !

● spectroscopy; ideally 1s 2s

- presently quantum state: n~30 !

-

--

-

CPT matter-antimatter

Page 76: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

Unique Ac DeceleratorUnique Ac

DeceleratorGatignon

Page 77: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

fibers77 K

BGO77 K

antiprotons

positronsource

positron traps

antiproton traps

rotating electrode

5.3 Teslamagnetic

field

4.2 K

Harvard: Trap, vacuum, rf electronics, … Juelich: Scintillation detectors

Small View

ATRAPATRAP

● trap and detectors

Gabrielse

Page 78: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

ATHENAATHENA

● annihilation of e+ and p-

- detects H

- insensitive to H velocity and state

-

-

Page 79: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

ASACUSAASACUSA

Balmer lines+ Qp/Mp TRAP@LEAR

Hayano

Page 80: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

Cooling before CaptureCooling before Capture

+ R&D developments

Hayano

Page 81: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

Precision Spectroscopy

Precision Spectroscopy

● antiprotonic spectroscopy

- large n

Hayano

Page 82: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

Improvements: ATRAP

Improvements: ATRAP

Status: 4.2 K antiprotons are routinely accumulated cooling thru matter

Improvements?• Needed: much lower temperatures• Desired: more antiprotons to speed data accumulation• Desired: more antiprotons to improve spectroscopy signal-to-noise

Decelerator? RFQD? ELENA?• would give the much larger antiproton rate desired• small ring would fit in AD hall• new beam lines would be needed• magnetic fields from experimental apparatus • substantial cost

Gabrielse

● new experimemts AEGIS ALPHA coming

Page 83: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

ELENAELENA

● A small machine for deceleration and cooling of antiprotons after AD to lower energies around 100 keV is feasible.

● One to two orders of magnitude more antiprotons can be available for physics.

● Main challenges for the low energy decelerator like ultra low vacuum, beam diagnostics and effective electron cooling can be solved, using experience of AD and member-state laboratories where similar low energy ion machines are operational (ASTRID, Aarhus; CRYring, Stockholm).

● The machine can be located inside of the AD Hall with only minor modifications and reshuffling of the present installation.

● Machine assembling and commissioning can be done without disturbing current AD operation.

Beloshitsky

Page 84: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

SPSCSPSC

● unique and leading p physics at CERN is foreseeable

● strong encouragement to continue > 2005

● improvements in beam switching highly desirable

● variety of different measureds for CPT desirable

● continue to explore improved trapping techniques- ELENA desirable- ELENA improvement on RFQD …… ?

● synergy between experiments always desirable

● roadmap should be updated and available

-

Page 85: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

7. Flavour Physics7. Flavour Physics

Ceccucci, IsidoriInagaki, LittenbergLourenco, Nakada

Sozzi, Tschirhart

Page 86: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

Flavour PhysicsFlavour Physics

●precision measurements of rare flavour decays probe the energy scale, and then flavour structure, of new physics- no SM tree- SM suppression- short distance dynamics

IsidoriMangano

FCNC

●experimental challenge BR~ 10-10 to 10-11

10% crucial for new LHC physics

Page 87: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

The ChallengeThe Challenge

theory uncertainty

Isidori

Page 88: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

LandscapeLandscape Mangano

Page 89: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

“NA48/3”“NA48/3”

~80 K+ πνν

● 2004launch GIGATRACKER R&Dvacuum testsevaluate straw trackerstart realistic cost estimationcomplete analysis of beam-test data

● 2005complete of the abovecomplete specificationssubmit proposal to SPSC

● 2006-2008construction, installation and beam-tests

● 2009-2010data taking

p io

n

NA48/3 COMPASS

Page 90: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

Beam:Present

K12(NA48/2)

New HI K+

> 2006Factor gainwrt 2004

SPS protons per pulse 1 x 1012 3 x 1012 3.0

Duty cycle (s./s.) 4.8 / 16.8 1.0

Beam acceptance H,V (mrad)

0.36 2.4, 2.0

Solid angle (sterad) 0.40 16 40

Av. K+momentum <pK> (GeV/c)

60 75 K+ : 1.50+ : 1.35

Total : 1.35

Momentum band pK (GeV/c)

Eff.: (p/p in %)

RMS: (p/p in %)

57 – 63 = 6 5 4

73.9-76.1=2.251.5

0.95

0.3750.30.25

Beam size (cm)Area at KABES (cm2)

1.5 7.0

2.5 20

2.8

Divergence: RMS (mrad) 0.05 0.1 2

high-intensity beam for K+→+ experiment

PRELIMINARY, WORK IN PROGRESS

Page 91: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

SPSCSPSC

● new rare decay frontier in K physics at CERN

● new experiments planned for Kπνν important

● support R&D now for K+π +νν results ≤ 2010- no competition … yet!

● longer term opportunity for K0π 0νν - direct competition (decay at rest)

● synergy with energy frontier @ LHC … @ CERN - B-physics - LF violation

● rare charm decay: feasibility of operating experiment (NA60) ?

Page 92: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

8. Other Projects8. Other Projects

Holzscheiter,IncagliUggerhodj, Zioutas

Page 93: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

MiscellaneousMiscellaneous

● CAST: astroparticle searches (from axions)best limits in window on axion mass

● AD4 p therapydosimetry and monitoring improving

● EM physics in crystalstrident production in critical field

●(g-2)μ : new experiment appropriateCERN pioneering pedigreeEuropean collaborators ?high intensity μ and ν evaluation

present CERN resource level appropriate

-

Page 94: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

9. Summary9. Summary

● fixed target physics at CERN

- ≤ 2011: physics vibrant, important, leading

SPS p.o.t ? schedule/prioritise/improve

completion of hadron program essential

CNGS window before T2K

hadron production for ν physics

ion+ion ≥ 2009 (synergy with LHC)

rare flavour ≥ 2009 (synergy with LHC)

fundamental physics with p atoms (+medical)

-

increasing p.o.t

Page 95: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

SummarySummary

All but HI benefit from/require high intensityRCPSB RCPS …

● fixed target physics at CERN

- > 2011: physics must be vibrant, important, leading

ion+ion ≥ 2009 (synergy with LHC) rare flavour ≥ 2009 (synergy with LHC)fundamental physics with p atomshadron structure: GPDs

dynamics: low energy, resonanceν physics: evaluation & R&D @ CERN

p-driver superbeam detectorglobal context NF

-… if appropriate ?

synergieswith otherscience?SPL?

Page 96: Villars 2004

John DaintonVillars 2004

October 7th 2004CERN seminar

ThanksThanks

“Always looking to the future, we pick up bad habits of anticipation.” Philip Larkin

to all who contributed toour deliberations