Title: Overview of the SLAC HEP Program
1Overview of the SLAC HEP Program
- Persis S. Drell
- Research Director
- SLAC
2(No Transcript)
3The SLAC Program
X-ray Experiments in FTTB
4B-Factory Program
5B-factory Program
- PEP-II Accelerator
- Collides e and e- with unequal beam energies at
ECM10.58 GeV - Premier tool for studying physics of heavy flavor
- BaBar Detector
- Optimized for B-physics at asymmetric energy
collider - Run by International Collaboration of gt 500
physicists from 74 institutions in 9 countries - Strong laboratory support for premier program
- Strong International Collaboration Leadership
- Spokesman Marcello Giorgi (Pisa/INFN)
- Analysis Coordinator Livio Lanceri (Trieste)
- Technical Coordinator Bill Wisniewski (SLAC)
- Computing Coordinator Stephen Gowdy (SLAC)
6USA California Institute of Technology UC,
Irvine UC, Los Angeles UC, Riverside UC, San
Diego UC, Santa Barbara UC, Santa Cruz U of
Cincinnati U of Colorado Colorado State Florida
AM Harvard U of Iowa Iowa State U LBNL LLNL U of
Louisville U of Maryland U of Massachusetts,
Amherst MIT U of Mississippi Mount Holyoke
College SUNY, Albany U of Notre Dame Ohio State
U U of Oregon U of Pennsylvania Prairie View AM
U Princeton U SLAC U of South Carolina Stanford
U U of Tennessee U of Texas at Albany U of Texas
at Dallas Vanderbilt U of Wisconsin Yale
Italy INFN, Bari INFN, Ferrara Lab. Nazionali
di Frascati dell' INFN INFN, Genova INFN,
Milano INFN, Napoli INFN, Padova INFN, Pisa INFN,
Roma and U "La Sapienza" INFN, Torino INFN,
Trieste Norway U of Bergen Russia Budker
Institute, Novosibirsk United Kingdom U of
Birmingham U of Bristol Brunel U U of Edinburgh U
of Liverpool Imperial College Queen Mary , U of
London U of London, Royal Holloway U of
Manchester Rutherford Appleton Laboratory
The BABAR Collaboration 9 Countries
74 Institutions 566 Physicists
Canada U of British Columbia McGill U U de
Montréal U of Victoria China Inst. of High
Energy Physics, Beijing France LAPP, Annecy LAL
Orsay LPNHE des Universités Paris VI et VII Ecole
Polytechnique, Laboratoire Leprince-Ringuet CEA,
DAPNIA, CE-Saclay Germany Ruhr U
Bochum Technische U Dresden U Rostock
7Building for the Future
Country Grad Students Post Docs BaBar PhDs
CANADA 6 3 0
CHINA 0 0 0
FRANCE 13 2 5
GERMANY 15 6 6
ITALY 25 13 4
NORWAY 1 0 0
RUSSIA 0 0 0
UK 27 20 14
USA 62 73 7
Totals 149 117 36
12/02
BaBar Physicist Members, Not Including Associates Underestimated people obtain permanent positions very early
8B-Factory Past Year
- 100 fb-1 (Run 2) followed by long (4.5 mo) down
- Shutdown work
- PEP-II
- Enable increased currents and smaller b
- BaBar
- TDC Upgrade for DIRC (French effort)
- SVT Work (Italy US)
- IFR Endcap upgrade (Italy US)
- Replace dying RPCs with efficient chambers which
have been carefully Q/Cd - Drift Chamber damage and repair
- Damaged during support tube extraction
- Full remediation within shutdown schedule
9B-Factory Past Year
- Turn-on November 15.
- Power spikes in December caused hardware damage
and run delays. - Running has now stabilized.
- Recent PEP-II Records
- Peak luminosity 5.21 x 1033 cm-2s-1
- Int. luminosity per 3 shifts 347 pb-1
- Total Luminosity Delivered 121 fb -1
10Analysis Improvements
- Steady improvements
- Better statistics
- Better understanding of detector
- In 2 years, CP measurement has moved from a test
of our understanding to defining our
understanding - Many ever more stringent tests yet to come
- CP violation in more complex decays
- Rare B decays
- Rich source of physics at least until the end of
the decade
sin2b 0.741 ? 0.067 (stat) ? 0.034 (syst)
11B-Factory Plans for Future
- Machine Luminosity Improvements
- Peak luminosity 7 x 1033 cm-2s-1
- Integrated luminosity 150/fb
-
- Peak luminosity 2 x 1034 cm-2s-1
- Integrated luminosity 500/fb
- Working on a path to
- Peak luminosity 4 x 1034 cm-2s-1
- Integrated luminosity 1-2/ab
- Detector Upgrades
- Begin replacing of Barrel IFR 2004
- Implement New Computing Model
6/03
2006
12Delivering on Promises
13The Competition
14Fixed Target Program
15SLAC 158
Parity-Violating Left-Right Asymmetry In Fixed
Target Moller Scattering
E158 Collaboration
- UC Berkeley
- Caltech
- Jefferson Lab
- Princeton
- Saclay
- SLAC
- Smith College
- Syracuse
- UMass
- Virginia
7 Ph.D. Students
16SLAC E158 Past Year
- Beam Delivery
- Run 1 23 April 27 May 2002
- Run 2 10 October 13 November 2002
- Run 3 7 July 31 August 2003
- Run I result announced 4/3/03
- Parity is violated in Møller scattering
- Limits on extra Zs at the level of 400-500 GeV
- Limit on lepton-flavor violating coupling 0.02
GF - Final results in 2004
17E158 Preliminary Results
APV-151.9 ? 29.0 ? 32.5 ppb
sin2?eff(Q20.025 GeV2) 0.2371 0.0025 0.0027
18Future of Fixed Target Program
- Real Photon Experiments
- Indefinitely delayed
- Future Fixed Targe Experiments in the Endstation?
- Depends on
- Physics Case
- Resources
19Linear Collider Program
20Linear Collider
- Exploration of the TeV scale will begin, but not
end with the CERN LHC - World-wide consensus (US, Europe, Asia)
- A high energy, high luminosity ee- linear
collider is the highest priority new project for
the field. - LC is the highest priority of the US HEP program
wherever it is built in the world. - US should bid to host this facility.
- It will not be built on the SLAC site
- SLAC has had ongoing program in machine (NLC) RD
- We are also working to grow a program of LC
detector RD
21Linear Collider Detector Effort
- Current focus on
- Ongoing simulations
- Currently looking at SD Silicon Tracker concept
for the LC detector - Under study here and elsewhere
- One of several approaches under consideration by
the community - Working to build effort at SLAC and provide
opportunities for user community to engage
22The SLAC Program
X-ray Experiments in FTTB
23Particle Astrophysics and Cosmology
24GLAST g-ray Large Area Space Telescope
- GLAST measures direction, energy and time of
celestial gamma rays from 20MeV 300 GeV - Collaboration of Particle Physicists and
Astrophysicists from France, Italy, Sweden, Japan
and US - Collaboration of Space and HEP funding agencies
from France, Italy, Japan and US - GLAST will survey the entire sky each day
- Active Galactic Nuclei
- Endpoints of Stellar Evolution Black Holes and
Neutron Stars - Dark matter
- Gamma Ray Bursts
- Discovery!
25GLAST/LAT Instrument
Si Tracker pitch 228 µm 8.8 105 channels 12
layers 2.8 X0 4 layers 18 X0 2 layers
Grid ( Thermal Radiators)
3000 kg, 650 W (allocation) 1.8 m ? 1.8 m ? 1.0
m 20 MeV 300 GeV
CsI Calorimeter Hodoscopic array 8.4 X0 8
12 bars 2.0 2.7 33.6 cm
Flight Hardware Spares 16 Tracker Flight
Modules 2 spares 16 Calorimeter Modules 2
spares 1 Flight Anticoincidence Detector Data
Acquisition Electronics Flight Software
- cosmic-ray rejection
- shower leakage
- correction
26GLAST
- Progress in Past Year
- Baseline CD-2/PDR in August 2002
- Good Technical Progress in all Sub-systems
- Project in transition from design to flight
hardware fabrication - Plans for Next Year
- CDR/CD-3 in May 2003
- Flight Hardware Fabrication
- Beginning of IT at SLAC
- On schedule for launch September 2006
27Other Particle Astrophysics
- Weekly particle astrophysics seminar series
- Continued analysis of USA data
- Studies of regions of strong gravity
- RD for new initiatives
- Ongoing projects using archival and guest
observer data - Experiments in FFTB and ESA
- FLASH (Next year)
- Lab Astro
- 2003 SLAC Summer Institute
28FLASH (E165)
- Uses the high energy electron beam to make
measurements of the fluorescence yield from
extensive air showers
- Goal 10 or better in energy of cosmic ray
29Kavli Institute
- Institute building on SLAC site
- Director reports to Stanford Dean of Research
- Operates as independent research center
- 9 new faculty
- Most (if not all) will be joint SLAC/Campus
- Director and Deputy Director recruited!
- Roger Blandford (CalTech)
- Steve Kahn (Columbia)
- Discussions beginning on the scientific
directions that the institute will take - It is anticipated the institute will bring in
funds from NASA and NSF that will flow through
campus in addition to DOE funds that will flow
through SLAC
30KIPAC
View from the entrance gate
View from the central lab
31Advanced Accelerator RD
32Advanced Accelerator RD
- Developing the tools that will define the future
of accelerator based science. - SLAC has a strong user driven program studying
physics of new acceleration mechanisms. - Laser-driven acceleration
- Plasma wake field acceleration
- Two beam acceleration
- Emphasis on proof of principle experiments
- Recent RD progress in breakout sessions
33Plasmas Have Extraordinary Potential
A 100 GeV-on-100 GeV e-e ColliderBased on
Plasma Afterburners
3 km
34ORION
FFTB 30 GeV e- e beams. New potential of e-
beams with sz lt 100 mm
ORION Facility (to be constructed in part with
funds from the ORION Center Proposal) based on
the NLCTA - 65 350 MeV e- beams
The initial use of the FFTB and subsequently
ORION facilities will allow a range of
experiments impossible elsewhere.
35RD for Future Experiments
36EXO Enriched Xenon Observatory
- Search for bb0 decay in reaction 136Xe --gt136Ba
e-e - Observation of decay would provide direct
evidence on - Lepton number violation
- Neutrinos are Majorana fermions
- Set neutrino mass scale
- EXO technique in RD phase
- Will hear about RD progress and future plans
(Rowson) - Successful RD would lead to full scale proposal
for EXO facility
37Theory Program
38SLAC Theory Group
- Primary mission to advance theoretical
high-energy physics, and to train young
scientists. - In addition, some members interact strongly with
the SLAC experimental program - Interests of the group span a range of extremely
challenging problems - Group well integrated with Institute for
Theoretical Physics at Stanford University - See many opportunities for interaction with KAVLI
Institute
39Computing
40Scientific Computing
- Data Driven Computing
- Large scale data management
- Driven by demands of BaBar
- Developing data management and GRID technology
that will be needed for LHC - Application Specific Computing
- Next generation accelerator modeling tools
- Large scale numerical simulations
- Positioned to support other applications
- Particle astrophysics
- Bio-molecular simulations
- .
41SLAC Long Range Planning Exercise
42Long Range Planning Exercise
- Scenarios for the Future of SLAC
- Develop models of SLAC as a partner in a future
LC under different assumptions - What might the ownership pieces of an LC be for
SLAC in various scenarios? - As we look towards our future, what are the other
exciting physics opportunities for SLAC to be
engaged in? - What is the physics case?
- Cost and technical difficulty?
- Consider which activities might be appropriate in
on-shore vs off-shore LC scenarios. - How do scenarios fit into an overall picture of
lab manpower and budget?
43Long Range Planning Exercise
- Process involves SLAC Staff, Faculty Users
- Chairs Tom Himel Persis Drell
- Goal Report to Director Fall 2003
Subcommittee A Raubenheimer (co-Ch) Paterson
(co-Ch) Brau Breidenbach Galayda Wolski Siemann Ro
ss
Subcommittee B Dixon (co-Ch) Seeman
(co-Ch) Burchat Colby Su Dong Hewett Jacobsen Kahn
Neal Schumm
44Summary
45The HEP Program at SLAC is focused on the central
issues of the field
- Pattern of heavy quark decays (B Factory)
- Electro-Weak Symmetry Breaking (Linear Collider)
- Physics beyond the SM
- Precision Electro-Weak (E158)
- Neutrino mass (EXO)
- Dark Matter, Dark Energy, Gamma Ray Bursts,
- Evolution of Early Universe (KIPAC, GLAST)
- Advanced Accelerator Techniques (FFTB, ORION)
- New Theoretical Frontiers
46The SLAC Program
X-ray Experiments in FTTB