an outlook from asia
DESCRIPTION
An Outlook from Asia. Atsuto Suzuki. Grenoble, July 27, 2011. Outline. 1. KEK Recovery Plan. 2. HEP Project in the Decades. 3. Quark Flavor Physics Project. 4. Lepton Physics Project. 5. Energy Frontier Project. 6. Non-Accelerator Physics Project. 7. Summary. - PowerPoint PPT PresentationTRANSCRIPT
An Outlookfrom Asia
Atsuto Suzuki
Grenoble, July 27, 2011
1. KEK Recovery Plan
2. HEP Project in the Decades
3. Quark Flavor Physics Project
4. Lepton Physics Project
5. Energy Frontier Project
6. Non-Accelerator Physics Project
7. Summary
Outline
1. KEK Recovery Plan
5/16
5/236/6
SuperKEKB
Sri Lanka:1
China: 12
Asia Korea: 11
UK: 11
EuropeCanada: 12
Americas
Universities
J-PARCwith JAEA
KEK
USA: 31
Australia:1
India:2
Malaysia:1
Taiwan:2
Ireland: 1
France: 11
Germany: 2
Italy: 4
Greek: 1
Swiss: 2
Poland: 4
Russia: 8Beraruce:1
Spain: 3
Georgia: 1Slovenia: 2
Bulgaria: 1Hungary: 1
Sweden: 1
Kazak stan: 1
Belgium: 1
Overseas Researchers ( 4/1~6/15): 133 (person), 1214 (person ・ day)
LANCE, RAL, PSI,ESRF, MAX, DIAMOND
APS, SSRL, ALS, TriumphSNS, FNAL, BNL, J-Lab,PNNL
NSRRC, SSRF, AS
Donation from CERN goes to orphans of the earthquake9 May 2011A donation of 53,280 CHF raised by employees and friends of CERN will go to Ashinaga, a non-profit organization which provides financial, educational and emotional support to children whose parents or guardians were lost or seriously injured as a result of the earthquake and the ensuing tsunami. The decision to donate to Ashinaga came after intimate discussion between Rolf Heuer, Director General of CERN, Atsuto Suzuki, Director General of KEK, and Shoji Nagamiya, Director of J-PARC. KEK would like to express our sincerest appreciation to those who support Japan, both in emotion ways and in terms of donations.
Daddy - Long - Legs
2008 2. HEP Project in the Decades
3. Quark Flavor Physics Project
∫L = 50 ab-1
J.P.Delahaye/CERN : ICHEP2010
Partially funded (100 M$)
Almost fully funded
30 M$ (2009) + 50 M$ (2010,2011,2012) + 100 M$ (KEKB for 4 years) + 30 M$ (overseas) +40 M$ (???) = 250 M$
350 M$
KEKB disassembling
Belle disassembling2014
SuperKEKB Collaboration
KOTO: K-Rare Decay at J-PARC
KOTO: K-Rare Decay at J-PARC
in May
BESIII data taking status & planPrevious Data set
BESIII Near future
J/psi BESII 58M 2009: 200M, 2012: 1 BPsi’ CLEO: 28 M 2009: 100MPsi” CLEO: 0.8 /fb 2010: 0.9/fb, 2011 2.5/fb(y 4040)/ (y 4160)
& scan CLEO: 0.6/fb @ (y 4160)
2011: 0.5/fb @ (y 4040)2013: 4/fb
R scan & Tau BESII 2014
BEPCII
BESIII data taking status & plan
Confirmation of BESII observation :X(1835) in J/ y gh’pp
New resonances in BESIII :X(2120) and X(2370)
in J/ y gh’pp
Confirmation of BESII observation :pp threshold enhancement
in J/ y decays
BESIII Collaboration
326 members, 46 Institutes, 10 Countries
274 members, 26 Institutes
8 members, 3 Institutes
9 members, 2 Institutes
3 members, 2 Institutes
1 members, 1 Institutes
5 members, 1 Institutes
4 members, 1 Institutes
11 members, 4 Institutes
1 members, 1 Institutes
10 members, 5 Institutes
4. Lepton Physics Project
T2K (Tokai to Kamioka) n Experiment
ne Event SelectionSelection Step events
There is no OD signal (fully contained: FC) 121In SK fiducial volume. (distance between reconstructed vertex and SK ID wall > 2m) 88One ring event 41e-like ring event 8Reconstructed electron energy > 100MeV 7There is no delayed electron signal from muons or pions. (to reject undetected muons and pions. ) 6Finding the 2nd e-like ring by forcing to fit to light pattern under the 2 e-like rings assumption, and then reconstruct invariant mass of these 2 e-like rings. Requesting Minv < 105MeV/c2; reject invariant mass close to p0 .
6
Reconstructed neutrino energy using the electron energy and direction is less than 1250MeV (E<1250MeV). Requesting that energy of neutrino is consistent with the one from J-PARC.
618
Beam intrinsic ne
NC p0 others Total (with error)
0.8 0.6 0.1 1.5±0.3Under the q13=0 hypothesis, the probability to observe six or more events is 0.007. (corresponds to 2.5 s stat. significance)
q13 measurements
• 90% confidence level region at d=0 case
Chooz experiment90% CL limit.
d= 0
(Dm232>0) (Dm23
2<0) MINOS
Collaboration
100m
300m
70m high
200m high
1,380m
290m
Far De-tector
Near De-tector
Reac-tors
YongGwang Nuclear Power Plant
~17 GW
Detector Construction & Closing (2011. 1)Detector Construction & Closing (2011. 1)
Near : Jan. 21, 2011
Far : Jan. 24, 2011
Completed RENO Detector (2011. 2) & LS ProductionCompleted RENO Detector (2011. 2) & LS Production
Liquid Scintillator Production System
DAQ Electronics
Control Room
* Sensitivity : sin2(2q13) > 0.02 Statistical errors (3 years of data taking with 70% efficiency)
Near : 9.83x105 ≈ 106 (0.1% error) Far : 8.74x104 ≈ 105 (0.3% error)
Systematic error : <0.5%
MINOS
• Data-taking is expected to start from August 1, 2011.
43 members, 12 Institutes, 2 Countries
T2K
Tunnel ( >3 km) construction finishedTest installation of module
Daya Bay Collaboration
293 members, 46 Institutes, 4 Countries
182 members (19 Institutes)
4 members (1 Institutes)
6 members (2 Institutes)
101 members (14 Institutes)
Sensitivity Sensitivity World q13 Race
RENO
Time is Money
Improve Precisionby 5 (0.1 ppm)
Improve Precisionby 100
Surface m
Muonium production(300 K ~ 25 meV 2.3 keV/c)
Ultra Cold m m Linac (300 MeV/c)
5. Energy FrontierProject
International Linear Collider
Test FacilityATF STF
ATF
S1-Global The first step of ILC2009 ~ 2011.2.25
Plug compatibility of SCRF system was successfully demonstrated by international collaboration.
Luminosity Increase of LHC using Crab Cavities
33
LHC Luminosity Upgrade
LHC Luminosity UpgradeIRQ Development
Required for Luminosity Upgrade
CLIC CLIC
breakdown probability /(m)
J.P.Delahaye/CERN : ICHEP2010
CLIC
Test FacilityATF
CLIC – ILC Collaboration
XMASSDark Matter Search:
Xe-loaded Sci.
High Scalability
1st 2nd 3rd
100 1 10 kg ton ton
6. Non-Accelerator Physics Project
KamLAND-Zenbb-Decay Search
Xe mixingXe extraction
EXO
SNO+ (56kg 150Nd)
MAJORANA
GERDA
1st step : 400 kg 136Xe
2nd step : 1 ton 136Xe (possible to 10 ton)
Jinping underground lab. of Tsinghua Univ. (2500m rock overburden)
Main Hall in June 2010
China Dark Matter Experiment
INO : India-based NeutrinoObservatory
50 kton magnetized iron module(s) with
30,000 channel RPC
1000 m
ToWorldport
7. Summary Nadeshiko
&