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26/01/05 A. Geiser, Discussion on T2K 1 program? benefits, options, and opportunities Introduction Outline of current questions in neutrino physics The T2K program Detector and schedules DESY-specific aspects Conclusions Achim Geiser ZEUS DESY group discussion on future opportunities 26. January 05

Participation in T2K neutrino program? benefits, options, and opportunities

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Participation in T2K neutrino program? benefits, options, and opportunities. Achim Geiser ZEUS DESY group discussion on future opportunities 26. January 05. Introduction - PowerPoint PPT Presentation

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Page 1: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 1

Participation in T2K neutrino program? benefits, options, and opportunities

Introduction Outline of current questions in neutrino physics The T2K program Detector and schedules DESY-specific aspects Conclusions

Achim Geiser

ZEUS DESY group discussion on future opportunities 26. January 05

Page 2: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 2

The T2K project

50 GeV p~1 GeV

Page 3: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 3

Assumptions on constraints

DESY contribution initially limited to manpower and resources as outlined in the HGF request

further contribution should be scalable both upwards and downwards, depending on resources and roadmap for DESY participation in ILC

need long term future option

individual DESY physicists cannot simultaneously participate in HERA and ILC and external activity (group can)

-> external activity in addition to declining HERA activity/stepping up ILC activity

Page 4: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 4

Current issues in neutrino physics

conservative assumption: neutrino oscillations are established! Super-K, SNO, KamLand + many others -> neutrinos have mass, (minimal) extension of Standard Model!

quark masses (6) and mixing parameters (4) are now all known; recently completed by CP violation parameters from Belle/Babar

out of the corresponding 10 mass and mixing parameters of the lepton sector (slide) , only 7 are (partially) known: me, m, m, m2

12, 12 („solar“), |m223|, 23 („atm“)

remain to be measured: absolute mass scale (tritium beta decay, double beta decay) sign of m2

23 mass hierarchy (slide) , matter effects

13 ! (~equivalent to Vub)

CP violation!!

Page 5: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 5

Current issues in neutrino physics

CP violation can only be measured if 13 /= 0 !

need 3-generation mixing!

Sign of m223 can only be measured if 13 /= 0 !

need e contribution! (matter effects)

leptonic CP violation might be able to explain baryon asymmetry in the universe (standard model instanton processes in Big Bang can turn lepton asymmetry into baryon asymmetry)

quark sector CP violation cannot (too small!)

measurement of 13 is very fundamental! T2K phase I

interest of CP violation is obvious T2K phase II + neutrino factory

Page 6: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 6

T2K (2009~)

K2K (1999~2005?)

Super-Kamiokande

40m250km

J-PARC@JAERI

CHOOZexcluded

sin2213

Sensitivity on e appearance

~20times

Neutrino physics at J-PARCTokai-to-Kamioka (T2K) LBL experiment

Off-axis sub-GeV beam from J-PARC 50GeV-PS

~3000 CC int./yr (w/o osc.) e appearance discovery disapp. precise meas. 5 year const. Start exp. in 2009.

S Nagamiya, NP04, KEK, August 24, 2004

Page 7: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 7

The T2K program

end of 2004: phase I finally approved!

2005-2008 prepare near detector,

reequip Super-K (far detector) with full phototube density

(1. April?) 2009: start data taking

(when they say april 1, they mean april 1)

measure/limit 13 ! (best sensitivity worldwide)

if /= 0, CP violation and matter effects can be large!

improve measurements of sin223 (=1 or not?) and m223

standard neutrino physics with near detector

in parallel, prepare for phase 2 (start 20xx?):

higher intensity beam (proton driver), intermediate detector, HK

Page 8: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 8

Location of JAERI at Tokai

TOKYO

KEK

JAERI

NARITA

KAMIOKA

Tokai

Tsukuba

S Nagamiya, NP04, KEK, August 24, 2004

Page 9: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 9

Replies to Recommendations (2)

Recommendation #3: The IAC strongly recommends that the neutrino oscillation experiment be brought into Phase I with additional supplementary funding. This would send a clear signal for international collaboration in this area. The neutrino project was approved for construction.

S Nagamiya, NP04, KEK, August 24, 2004

Page 10: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 10

Construction Schedule

Linac

3 GeV

50 GeV

Materials + Life

Nuclear-Particle

Neutrino (plan)

Others

Salt Farms

Bldg. construction

Equip. constructionBeamtest

Bldg. construction

Equip. constructionBeamtest

Bldg. construction

Equip. constructionBeamtest

Bldg. construction

Equip. constructionBeamtest

Bldg. construction

Equip. constructionBeamtest

Bldg. construction

Equip. constructionBeamtest

Construction

Archelogical studies

Construction Schedule (as of Oct., 2003)

FY2001 FY2002 FY2003 FY2004 FY2005 FY2006 FY2007 FY2008

BeamConstruction Start

study report

1) Budget and Schedule

S Nagamiya, NP04, KEK, August 24, 2004

Page 11: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 11

Expected Beam Power

Beam Test

0.2

0.0

MW

1.0

0.8

0.6

0.4

JFY2007

平成23年度 平成24年度平成19年度 平成20年度 平成21年度 平成22年度

Usage for Experiments

Usage for Experiments

Usage for Experiment

3 GeVNeutron and Muon Construction

Construction

Construction

KEK PSPower

Completion of200 MeV Linac

400 MeV Linac Construction

200 MeVon Day 1

Expected Beam Power at 3 GeV

400 MeVon Day 1

400 MeV installationin 2008-2010

JFY2008 JFY2009 JFY2010 JFY2011 JFY2012

Completionof T2K

50 GeVNuclear - Particle

T 2 K Experiment

1) Budget and Schedule

S Nagamiya, NP04, KEK, August 24, 2004

Page 12: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 12

IAC, March 2004

2) Construction Status S Nagamiya, NP04, KEK, August 24, 2004

Page 13: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 13

3 GeV Quadrupole Magnet 2) Construction Status

S Nagamiya, NP04, KEK, August 24, 2004

Page 14: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 14

Letters of Intent for 50 GeV

Announce of LoI call : July 2002 Thirty LoI’s were submitted by early 2003

Strangeness nuclear physics 7 Nuclear/hadron physics 7 Kaon decay physics 4 Muon physics 3 Neutrino physics 1 Future facilities 8

478 physicists with 2/3 from outside Japan. Asian participation is still few.

Call for proposals: Most likely, within half(?) a year, if no further delay is observed for the 50 GeV construction.

Nuclear/Particle Facility LOI Authors

Total #= 478

Japan

North America

Europe

Asia

4) Letters of Intent

S Nagamiya, NP04, KEK, August 24, 2004

Page 15: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 15

Timeline for 50 GeV Proposals

2003 2004 2005 2006 2007 2008

NowBeam

Final Decision onDay-1 Experiments

Call forProposals

Formation of PAC

Discussionof LoI's

Current Issue before the formatin of PAC: Organization at the Operational Stage

S Nagamiya, NP04, KEK, August 24, 2004

Page 16: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 16

From K2K to T2K

T2K = Tokai to Kamioka(not yet an official name)

e

AtmosphericNeutrino

K2K,MINOS,CERN T2K

Atmospheric neutrinoAccelerator neutrino

Solar neutrinoReactor neutrino

+

KamLAND+

SNO

Best fit

Flux () at J-PARC 50 GeV PS > 100 x Flux () at KEK 12 GeV PS

With oscillation

Without oscillation

Data since 1999K2K = KEK to Kamioka

108 eventsobserved(151 events expectedwithout anyoscillations)

99.99% confident that carries a finite mass.

3) Recent News in Sciences

S Nagamiya, NP04, KEK, August 24, 2004

Page 17: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 17

e appearance.

Overcome the background and correctly estimate the remaining background. sin22e=0.05,

m2=3×10-3eV2

mostly 0

mostly from decay

LOI

Page 18: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 18

Conceptual Off-Axis 280m Detector

Magnet (and side MRD)

Magnet (and side MRD)

Electron calorimeterFine Grained detectorw/ or w/o water target Scintillator

Tracker (TPC or chambers)Iron shield for -ID

Page 19: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 19

UA1 Magnet

7.64(L)× 6.116(H)× 5.596(W) B=0.67T (UA1), 0.4T(NOMAD),

≤0.2T (T2K for power<0.6MW) NOMAD experiments

Page 20: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 20

Instrumenting the iron

“C” are made of plates of iron 4.8 cm thick Gap of 1.7 cm between plates It is possible to insert scintillators in the gaps (1 complete layer ~ 90 m2) (extruded scintillators with fibers?)

For UA1 = hadron calorimeter For T2K = muon range detector

Page 21: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 21

Full Active target detector

SciBar-like to measure the exclusive final states.

Page 22: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 22

T2KInterim Collaboration Agreement

andInterim MoU for the Common Project

which are under discussion in the IBR

K. Nakamura, T2K collaboration meeting, 24.8.04

Page 23: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 23

Interim Agreement on International Collaboration

K. Nakamura, T2K collaboration meeting, 24.8.04

T2K Collaboration does not have a Collaboration Agreement yet.

In the formal CA, we (Spokesperson + KEK Representative) wish to specify contributions from each participating Institution/Country/Region to the Experiment.

Until the funding situation of most of the participating Institution/Country/Region becomes clear, we wish to proceed with an Interim Agreement.

Until the formal CA is signed, the IBR (International Board of Representatives) functions as the Executive Committee.

Organization, Institutional Responsibilities, Membership, etc. will be defined.

Page 24: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 24

T2K Interim Board of Representatives

Spokesperson K. Nishikawa

Construction group representative T. Kobayashi

National / Regional representativesCanada A. Konaka, J.M. Poutissou

Italy M. Mezzeto France F. Pierre

Korea S.B. Kim Poland D. Kielczewska

Russia Y. Kudenko Spain E. Fernandes

Switzerland A. Blondel UK D. Wark

USA G. Beir, C.K. Jung*, H. Sobel

KEK representative K. Nakamura

ICRR representative Y. Suzuki

K. Nakamura, T2K collaboration meeting, 24.8.04

Page 25: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 25

Common Project and Common Fund for Facilities Related to Neutrino Beam and Near Detector

As one of the host institutes of the T2K Experiment, KEK is responsible for the civil construction of the facilities related to the neutrino beam and the near detectors.

The construction of the neutrino beam line and the near detectors including part of the beam extraction system is defined as the Common Project of the T2K Collaboration.

Each collaborating Institute/Country/Region is expected to contribute to the Common Project appropriately.

Contributions to the Common Project will be made in two ways: In-kind contribution to supply engineering work and/or equipments cash contribution to the Common Fund

KEK as a host institute will exchange an Interim MoU with each contributing Institution/Funding Agency with regard to funding request for the contribution to the Common Project.

When funding is allocated, the Interim MoU will be replaced with the MoU between KEK and the contributing Institution/Funding Agency.

Page 26: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 26

potential DESY participation? disclaimer: the following is an example for a hypothetical scenario made up by me, not

yet discussed with the DESY management nor with the T2K collaboration

phase 0: 2005/6? main hardware/software/analysis activity: HERA convergence towards decision on external DESY participation preparation of potential bilateral german-japanese agreements discussion on agreement at European level to become part of a European hub for infrastructure (hardware, test beams, meetings) and computing/analysis

for test beam and physics data collaboration agreement on detector tasks and access to far detector data, in-kind contributions? (beam-line elements (HERA), detector parts (ZEUS)) formally join T2K collaboration in 2006?

phase 1: 2007/8? main analysis activity: HERA work on hardware/software contribution to T2K

detector construction activities according to agreement electron test beam activities, including support for other European groups preparation of online and monitoring software preparation of analysis software

Page 27: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 27

potential DESY participation? phase 2: 2009-final ILC approval? start of T2K data taking shift of analysis activity HERA -> T2K hardware activity towards intermediate+far detectors?

running in of near detector participation in data taking shifts start European or European/US analysis activity! (attract students) prepare participation to T2K stage 2 (e.g. intermediate detector, HK) in parallel after end of HERA analysis: participate in ILC+detector design

activities (e.g. T2K diploma students -> ILC PhD students)

phase 3: ILC approval-ILC startup? main analysis activity: T2K rescale hardware/software contribution to T2K for compatibility with ILC+detector plans

data analysis! (oscillations + many „standard“ physics topics) define scale of participation to T2K phase 2 hardware depending on available

resources continue role as infrastructure provider in any case (=minimum involvement)

Page 28: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 28

Conclusions

DESY participation in T2K would offer great physics opportunities (attract students + postdocs) fit transition time between end of HERA analysis and start of ILC analysis offer opportunities to collaborate with German and European partners in a fully international project and serve as a German or maybe even

European Hub offer opportunities for application of expertise in particle physics analysis,

detectors and beam line elements (+ in-kind contributions from ending HERA program??) allow to participate with initially limited resources allow to scale future hardware commitments according to ILC

developments offer excellent long term perspectives, if wished, via an intermediate

detector and a Megaton far detector towards a neutrino factory

If participation to an external project is considered at all, this option ideally matches all the requirements

Page 29: Participation in T2K neutrino program?    benefits, options, and opportunities

26/01/05 A. Geiser, Discussion on T2K 29