THE STATUS of BABAR Marcello A. Giorgi Università di Pisa /INFN/SLAC 11/21/2002 Marcello A.

Download Report

Transcript THE STATUS of BABAR Marcello A. Giorgi Università di Pisa /INFN/SLAC 11/21/2002 Marcello A.

THE STATUS of BABAR
Marcello A. Giorgi
Università di Pisa /INFN/SLAC
11/21/2002
Marcello A. Giorgi
1
OUTLINE
•
•
•
•
Down period and detector activity
Ready to startup
Physics Analysis
Toward future achievements
11/21/2002
Marcello A. Giorgi
2
Down period Activity
(DETECTOR)
• The main and programmed activities on the BABAR
Detector:
– the intervention on the IFR End Cap (muon/KL
detector ).
– The installation of new TDC in the Dirc .
– The maintainance of SVT (possible because of the
extraction from BABAR of Support Tube containing
SVT, beam pipe and magnetic elements of interaction
region)
11/21/2002
Marcello A. Giorgi
3
IR2 Schematics
11/21/2002
Marcello A. Giorgi
4
DCH damage and repair
•
On July 31, during removal of
the support tube, a bolt head
cracked the DCH Be inner
cylinder.
11/21/2002
Marcello A. Giorgi
5
DCH Damage and Repair, Summer 2002
"
"
"
"
"
"
Support tube hit inner cylinder
6" x 1" crack in beryllium section
No environmental contamination
IC still about 7x structural load
Filled with epoxy
Covered with Al
"
"
"
"
11/21/2002
Helium tight (< 50 ml/min)
Electrically grounded
5 mm clearance to support tube
No damage to nearby wires
Marcello A. Giorgi
6
SVT work
SVT has been un-cabled,taken to the clean room, split in two
halves and removed from the B1 magnets
•Once the SVT was exposed electrical tests and visual inspections
were performed. We discovered the reason for some of the
failures of the 9 non functioning readout sections,some modules
fixed!
•
11/21/2002
Marcello A. Giorgi
7
SVT Recovered Sections
Rotated
Tail
Slipped
Milpac
11/21/2002
Fixed
Sections
Marcello A. Giorgi
8
SVT & Support Tube Installation
11/21/2002
Marcello A. Giorgi
9
DIRC shutdown main activity: TDC upgrade (I)
Issue: background rate versus luminosity:
expectation: rate (kHz) ~ 530 at L=4. 1034
cm2/s
high inefficiency with current design
 New TDC design to allow small dead time up to 1 MHz rates
11/21/2002
Marcello A. Giorgi
10
DIRC shutdown main activity: TDC upgrade (II)
TDC chips: 12 (sectors) × 14 (Front End Boards) × 4 (chips)=672
Sector crate
Boards: - removed and sent to external company for chips exchange Front end board
- re-coded and tested in test bench at SLAC
- re-installed in detector
and fully tested with calibration data: OK
October 11th 2002
TDC upgrade successful !
11/21/2002
Marcello A. Giorgi
11
DIRC cosmic data
Occupancy: hit frequency per phototube
Typical distribution for cosmic data
Timing distribution also look very good
11/21/2002
Marcello A. Giorgi
12
IFR Forward Endcap
The improvement in the Forward Endcap
• REPLACEMENT OF RPC
• Insertion of BRASS to increase absorber thickness
• ADDITIONAL LAYER 18&19 (double gap)
• ADDITIONAL BELT around Endcap
• New gas system
• New HV distribution
11/21/2002
Marcello A. Giorgi
13
New Forward EndCap project
RPC belt
Terminology:
19 slots
and 15 RPC layers
Slot18/19
5 brass layers
(slot 8,10,12,14,16)
Absorber Segmentation
7 layers 2 cm
1 layer 7 cm
2 layers 9 cm
2 layers 13 cm
2 layers 10cm
11/21/2002
Marcello A. Giorgi
total 85 cm
14
GT/SLAC cosmic test
All the RPC
with maximal
efficiency
• Cosmic test at RPC producer General Tecnica and SLAC
– QA test
» Gas leakage test before and after shipping
» Dark current
Radiography
HV Plateau
Strip Occ.
96%
HV [V]
11/21/2002
Marcello A. Giorgi
15
Barrel IFR Upgrade
Decreasing efficiency
Some RPC completely off
The problem: dying RPCs.
Muon selectors
losing efficiency
impacting physics
11/21/2002
Marcello A. Giorgi
16
Barrel IFR Upgrade
• We are now in the middle of the process to understand the
best way to fix this problem. ‘Remediation’ has not been a
success.
• Working committee formed to recommend an upgrade
technology. There are three candidates: improved RPCs with
better Q/C, Limited Streamer Tubes, and Scintillator read
by APDs.
• Decision expected by January.
• Access for replacement of current RPCs is mechanically
complex: significant engineering needed. Expect to upgrade in
2004 and 2005 to avoid an extremely long shutdown.
11/21/2002
Marcello A. Giorgi
17
Trigger
L1 Trigger:
L3 Trigger:
1.1khz @ 4x1033
Output 130Hz @ 4x1033
Software trigger executes on 47 Linux farm nodes (1.4Ghz Pentium-III
dual CPU with Gbit Ethernet, recently replaced 60 Sun Ultra-5 nodes).
L3 algorithms run at ~4ms/event.
Trigger Strategy:
Goal:
Trigger on physics with high, stable and measurable efficiency.
Strategy: Orthogonal tracking and calorimeter triggers with high
efficiency at both L1 and L3 for most physics sources.
Efficiency: Total: eBB>99%, eudsc~97% Fiducial: eee,mm>99%, ett~92%.
11/21/2002
Marcello A. Giorgi
18
Level-1 Drift-Chamber Trigger Upgrade
Need to contain L1 rate to <3 Khz at future high luminosity running to avoid DAQ
bottleneck in DCH frontend data shipping.
Z information needed, therefore
the tracking trigger must be
redesigned
The upgrade task:
24 Track segment finders (TSF)
8 Z-Pt-Discriminators (ZPD)
33 Interface boards of 3 types
All boards in prototyping phase.
Expected production in Jan/03.
Commissioning starts Mar/03.
ZPD prototype (9U VME):
XilinX Vertex II 3000/4000 FPGAs.
120MHz databus & internal logic.
11/21/2002
(will run new system in parallel
to exisitng system initially
with DCH trigger fiber signal
splitting).
Marcello A. Giorgi
19
COMPUTING
Event Data Flow
Analysis
Skims
HPSS
Objy
Oep
PrompReco
Ntuple
SimProd
Root
Production
11/21/2002
Marcello A. Giorgi
20
Computing Model Discussions
• Current Model defined in 2000 (April review suggested an update)
• BaBar has 4 Tier-A sites (France, Italy, UK, US)
– New German centre (probably) next year
– Looking at how to best utilise these distributed resources (BaBar
GRID is one tool for this)
• Multiple analysis formats (now)
– Objectivity, ROOT and Ntuples
– Multi-step process
– Problems found at any level need fixes propagated to other formats
• A committee is currently considering the computing model
with increased luminosity within a limited resource scenario
(in both people and money)
• Attempting to replace all three with ROOT
– Ntuples will still be needed, but to a much lesser extent
• Report will be internally reviewed on December 6th, 7th
11/21/2002
Marcello A. Giorgi
21
BaBar Physics Analysis
Initial targets for PEP-II and BaBar:
25 ICHEP’02
New environment: high luminosity asymmetric collider submissions
Search for CP violation in B mesons decays: found !
Establish methods for precision B physics, rare B decays
some highlights
on Run 1 + Run 2
Journal publ.
in preparation
What next? Discovery potential
Probe CKM model  new physics ?
Active analysis
Rare decays, searches (not only B)  new physics ?
subjects (2)
Along the way: constrain heavy quark models
11/21/2002
Marcello A. Giorgi
22
CP violation: sin2
hcp=-1
hcp=+1
sin2 = 0.755  0.074
sin2 = 0.723  0.158
sin2 = 0.741  0.067 (stat)  0.034 (syst)
hep-ex/0207042, Submitted to PRL
11/21/2002
Marcello A. Giorgi
23
CP discovery
in B sector
Osaka -2002
Rome- 2001
Amsterdam- 2002
11/21/2002
Marcello A. Giorgi
24
Towards sin2eff
B0 → + 

ACP
= -0.22+-0.08
0.08 ( stat )  0.07( syst )
C   = 0.45+-0.18
0.19 ( stat )  0.09( syst )
S  = 0.02  0.34( stat )  0.05( syst )
C  = -0.30  0.25( stat )  0.04( syst )
11/21/2002
B0   
S   = 0.16+-0.25
0.25 ( stat )  0.07( syst )
Marcello A. Giorgi
25
Semileptonic B Decays and |Vcb|
Fit to sum of spectra from:
B  D e n, D* e n,
D** e n, D(*)  e n
BR(BX e n) = (10.87 0.18stat 0.30sys)%
|Vcb| = 0.0423 0.0017exp  0.0020theory
11/21/2002
Marcello A. Giorgi
Integration over spectrum &
extrapolation to pl*=0
Relation to |Vcb| by
Hoang-Ligeti-Monahar
26
Penguins and rare b decays
B(B  XS ) = (3.88  0.36(stat)
EM
54.6 fb-1
0.43
 0.37(sys) +-0.23
(theory)) 10-4
Exclusive measurements:
also interesting for |Vtd/Vts|2
EW
85M BB pairs
BB     1.9 106
90% C.L.
BB    BB  K *   0.047
+ 0.11
-6
B(B  Kl+ l - ) = (0.78+-0.24
)

10
0.20- 0.18
-6
B(B  K *l + l - ) = (1.68+-0.68
0.58  0.28)  10
 3.0 10 -6 @ 90% C.L.
QCD
B
11/21/2002

BF B

 60106 B pairs
BF B   K * = 9.2  1.0  0.810-6
K0
S
51 events
0
 + 1.7

 K S0 =  8.7
 0.9  10-6
 - 1.5


sin 2 = - 0.19+-0.52
0.50 ( stat )  0.09( syst )
Marcello A. Giorgi
27
What next? Probe CKM in detail…
sin2 uncertainty still far from systematic limit
Several modes can give information on each side and angle
All actively analyzed in BaBar. Key element: integrated luminosity!
B0, 

buln
B(,,) ln
*
VudVub
BDK
B K,  
11/21/2002

*
B0 Mixing
B(,) 
VtdVtb
*
VcdVcb
bcln
Marcello A. Giorgi

B0y,,h KS
B0D(*)+D(*)28
…and with higher and higher luminosity:
Rare B decays, for instance:
Loop-mediated, FCNC: b  sl+l-, b s nn, b  s
Leptonic: B  tn, …
Unique possibility at B factories: fully reconstructed B tag
 0.1% efficiency, very useful for channels with missing energy (n)
Just began to exploit this possibility
Charm and Tau Physics
Search for mixing and CP violation in D meson decays, …
Rare t decays, including LFV
11/21/2002
Marcello A. Giorgi
29
BABAR back again and READY !!
• After the down period BABAR is ready to take
data in better shape than in the last July
• We are ready for higher luminosity with hardware
and software
• We have an exciting Physics Program beyond the
original scientific mission
• We are prepared to improve our muon detection
(the technology of the barrel IFR will be chosen in
January 2003)
• We continuously monitor our computing model to
improve it and to make our Physics Analysis more
effective
11/21/2002
Marcello A. Giorgi
30
Hadronic event from OPR
Nov.18,2002
11/21/2002
Marcello A. Giorgi
31
Preliminary from task force on Long
Term Upgrades
The task Force will deliver soon the written report to the collaboration
Some Highlights:
BABAR is a pretty good detector: very difficult to improve
it!! (IFR is the only intervention needed)
Only a few channels are systematically limited below 1 ab-1 ;
many topics would benefit from 2-3 ab-1 or more
We need to integrate higher luminosity, well beyond 0.5 ab-1,
to better constrain the Unitarity triangle, to study rare
decays and try to open windows on New Physics.
More resources to PEPII would be beneficial for Physics
11/21/2002
Marcello A. Giorgi
32
The enthusiatic people of BABAR
11/21/2002
Marcello A. Giorgi
33
BACKUP
11/21/2002
Marcello A. Giorgi
34
SVT Split
11/21/2002
Marcello A. Giorgi
35
SVT Current Status
• In July 9/208 readout sections were not working.
NOW:
• 3 of them fixed.
• 3 read-out sections still under investigation
• 3 can not be fixed:
• No new non functioning read-out section has been introduced.
• We lost redundancies on 2 modules
11/21/2002
Marcello A. Giorgi
36
Barrel repair
•Four major activities
–New HV distribution
•Replace plastic boxes
•FEC fixing
•Major failure in Feb 2002
–Gas distribution
•Remote monitoring
–RPC remediation
•Try to increase RPC eff
by accumulating charge
11/21/2002
Marcello A. Giorgi
37
Computing Online
• Replaced initial Solaris farm
– Installed in 98/99
• 50 Linux machines
– Extra capacity to cope with increased luminosity
– Allows better rejection of background in Level 3
11/21/2002
Marcello A. Giorgi
38
Preliminary report from the Task
Force on “Long Term Upgrades”
Roy Aleksan and David MacFarlane have reported
last September 2002 at the collaboration meeting
held London on the activity of the Task Force set
in December 2001.
The final report is expected soon.
Meanwhile some important considerations can be
extracted from the evaluation of the task force.
11/21/2002
Marcello A. Giorgi
39
From task Force
• PEPII&BABAR have met their CHALLENGE. So far
machine and detector have operated very well,
beyond what anticipated
• No limitation for many modes from systematic
effects up to 0.5 ab-1 and for many other
channels up to 2-3 ab-1, it will allow us to pursue
new goals toward a comprehensive study of CP and
search for new physics.
• But many topics as Vub,Vtd with ,  and  with 
() DK (DK) rare decays (penguins), non b
physics will benefit (they need) from higly
increased statistics.
11/21/2002
Marcello A. Giorgi
40
From task force
• BABAR is a pretty good detector and it is very
difficult to improve it significantly
• Some gain for  (similar or better for ),but non
overwhelming in improving SVT by adding an extra
layer at a smaller radius. The intervention is
technically difficult and the risk in reducing beam
pipe diameter to 20mm or less could imply high and
unquantified operational risk.
• A forward veto calorimeter integrated with a
modified B1 looks feasible for 2005, but we could
not identify so far a significant gain for Physics.
11/21/2002
Marcello A. Giorgi
41