fermilab program overview pier oddone september 25, 2007
TRANSCRIPT
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Fermilab Program OverviewFermilab Program Overview
Pier Oddone
September 25, 2007
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Transition completed successfullyTransition completed successfullyL.8 Offeror’s Involvement/Resources
Clearly defined responsibility for corporate oversight
Robert Zimmer, ChairFred Bernthal, Vice-
ChairPier Oddone,
President
Robert Zimmer, President
Fred Bernthal, President
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ProgramsPrograms
The Energy Frontier Tevatron, LHC ILC, LHC Upgrades
The neutrino frontier Minos, MiniBooNe, SciBooNe NOvA, Minerva
Particle Astrophysics SDSS, Pierre Auger, CDMS II DES, CDMS-25kg, SNAP
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Program featuresProgram features
Theory and Computation Play a key role in all three aspects of the program
Collaborations From the beginning an NTF: True National Laboratory New consolidation of facilities at Fermilab –>> increased
responsibility
Planning for the future Critical juncture for particle physics Plans developed with the HEP community
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Tevatron: the fuelTevatron: the fuel
Tevatron peak and integrated luminosities
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Tevatron: the productTevatron: the product
Very large number of results – dominant at international conferences
Important constraints from precision measurements, direct searches, rare decays
The laboratory and collaborations’ position: extend running through 2010.
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Constraint MSSM (CMSSM)Constraint MSSM (CMSSM)
Sven Heinemeyer, Georg Weiglein
With Electroweak precision measurements and cold dark matter density (WMAP, …)
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SM Higgs Searches at TevatronSM Higgs Searches at Tevatron
Tevatron Observed
Tevatron Expected
LP2007LP2007
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LHC CommissioningLHC Commissioning
Major problem with inner triplets in March test
All triplets are fixed, several pressure-tested in the tunnel, most installed
Root cause analysis is complete and available on the web
Sector 4-5 may have to be warmed up for triplet installation
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LHC Commissioning: inner tripletsLHC Commissioning: inner triplets
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LHC Commissioning: timelineLHC Commissioning: timeline
June
12
sche
dule
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Commissioning: Remote Ops. CenterCommissioning: Remote Ops. Center
LHC AcceleratorLHC Detector (CMS)
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CMS CommissioningCMS Commissioning
Established CMS Center, headed by Lothar Bauerdick
New leadership in LHC Physics Center: Dan Green and Chris Tully
Commissioning detector underground
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CMS CommissioningCMS Commissioning
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ILC preparationsILC preparations
Major development of infrastructure at Fermilab NML Cryomodule Test Facility IB-9 Clean Room Facility With ANL: EP and BCP processing facility Vertical Test Stand Horizontal Test Stand
Key player in the RDR and EDR in collaboration with many institutions
Central role in linac SCRF technology development and conventional/site studies
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ILC preparationsILC preparations
Vertical Test Stand
Horizontal Test Stand
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ILC preparations: NMLILC preparations: NML
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ILC preparationsILC preparations
3.9 GHz Cryomodule Clean Room Cryomodule assembly
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Neutrinos: MiniBooNENeutrinos: MiniBooNE MiniBooNE rules out to 98% CL the LSND result interpreted as e
oscillations described with standard L/E dependence
The as-yet-unexplained deviation of MiniBooNE data from prediction at low-energy Under investigation
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MC
MINOS MC
SuperK
By 2009
K2K
MINOS 2007
Neutrinos: MINOS sinNeutrinos: MINOS sin22222323 + + mm
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Neutrinos: expanding programNeutrinos: expanding program
Minos: search for electron appearance
MiniBooNE: what is happening at low energy
SciBooNE (from K2K detector) running well
Minerva construction started
NOvA project start; CD2/3a this November
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On-site reviewOn-site review
Particle Astrophysics: SDSSParticle Astrophysics: SDSS
As seen in: National Geographic, Hoshi Navi and Newton (Japanese magazines), and soon in a college-level Chemistry textbook (Silberberg)
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This plot shows constraints on cosmological parameters from SDSS galaxy distribution. Yellow and orange are WMAP [1 year and 3 year]; red is adding in SDSS. Notice how constraints on w and neutrino mass are especially tightened by SDSS.
SDSS: combined results WMAPSDSS: combined results WMAP
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CDMS Running at SoudanCDMS Running at Soudan
Current sensitivity of CDMSXenon10 limitPublish
ed CDMS limit
DAMA MSSM
~650 kg-day exposure
Large calibration data sets
High efficiency for collecting data
CDMS is the only direct detection dark matter experiment currently running without backgrounds!
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Pierre AugerPierre Auger
Hybrid event (~1019eV) recorded by four fluorescence telescopes and the surface array
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Pierre Auger: Energy spectrum Pierre Auger: Energy spectrum
Calibration unc. 18%FD syst. unc. 22%
5165 km2 sr yr ~ 0.8 full Auger year
Exp Obs>1019.6 132 +/- 9 51
> 1020 30 +/- 2.5 2
Suppression evident at high energy
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Additional impounded resultsAdditional impounded results
Remarkable first result from COUPP. Submitted to Science
Exciting results on the origin of ultra-high energy cosmic rays from Pierre Auger. Submitted to Science
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Major issue: planning for the futureMajor issue: planning for the future
What is the national program: especially the accelerator based domestic program?
Planning has to be centered on recovering the energy frontier: ILC
But there are unresolved issues Sufficient energy at 0.5 TeV? Domestic and international arrangements? When?
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Problems with competitive situationProblems with competitive situation
In a world with a delayed ILC or no ILC – grave risk that we are left ONLY with accelerator R&D without world leading facilities either at the energy frontier or the intensity frontier
Once we are in that bucket: much harder to get out to a position to build the next global facility: the accelerator based program will be smaller
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Problem: selection vs. roadmapProblem: selection vs. roadmap
We have selected the projects to start: DES, NOvA, Daya Bay – only NOvA is a “large project”. It is the start of a roadmap
Problem: “…I want a dialog with the HEP community…” leads to “we’ll talk to you in three years….”
Example: can say “wait until we know sin213” or build a roadmap that depends on that number
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Fermilab Steering GroupFermilab Steering Group
Steering Group NOT to provide a plan A vs. plan B, rather an integrated roadmap with discovery opportunities in the next two decades that:
supports the international R&D and engineering design for as early a start of the ILC as possible and supports the development of Fermilab as a potential host site for the ILC;
develops options for an accelerator-based high energy physics program in the event the start of the ILC construction is slower than the technically-limited schedule; and
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Fermilab Steering GroupFermilab Steering Group
includes the steps necessary to explore higher energy colliders that might follow the ILC or be needed should the results from LHC point toward a higher energy than that planned for the ILC
Broad community engagement under the leadership of deputy director Young Kee Kim
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What we are asking P5What we are asking P5
Take into consideration it takes a minimum of four years to break ground on any new project
Need recommendations on the roadmap that take account of the full complexity of the world in which we live
If the roadmap we propose is to be effective, it needs R&D support for project preparation