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FNAL

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Fermi Research Alliance was awarded the contract to operate Fermilab for 5 years ... All Experimenters' Meeting at 4 pm TODAY Curia II. October 27,28, 2006. 7. f ... – PowerPoint PPT presentation

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Title: FNAL


1
  • FNAL
  • Hugh Montgomery
  • Fermilab
  • October, 2007

2
Organisation Issues
  • Fermi Research Alliance was awarded the contract
    to operate Fermilab for 5 years with possibility
    of up to 20 years, if performance is good.
  • FRA is partnership between U. Chicago and URA.
  • FRA Board of directors, Chair is Bob Zimmer,
    President of U. Chicago.
  • Board has 7 URA regional representatives
  • Physics Sub-committee still exists and they
    organize a Physics Visiting Committee review.

3
Organisation Issues
  • FY2008 Budget As last year there is a Continuing
    Resolution, so the year starts as a continuation
    of last year, No new starts, no increases for
    projects on the rise.
  • Divisions and Sections had a preview in July but
    we have not distributed a strawman budget, nor
    heard responses.
  • In DOE OHEP, Robin Staffin has moved on to be an
    advisor to Ray Orbach, OHEP has Acting Head,
    Dennis Kovar, who was Head of Nuclear Physics for
    many years.
  • We are developing a budget briefing for Dennis
    for Wednesday, October 31.

4
Long Range Planning
  • Steering Group
  • Chair Deputy Director -Young Kee Kim
  • Committee 50/50 Fermilab-Non Fermilab
  • Plan US Accelerator Based Future supporting ILC
  • Report in September 2007
  • If ILC decision is delayed
  • Build 6 GeV ILC Linac
  • 2 GeV LINAC front end
  • Feed 8 GeV to Accelerator complex and physics
  • Eg gt 2 MW for 120 GeV protons for LBL Neutrino
    Program
  • 8 GeV protons for muon and kaon program
  • Recommendations are under discussion by everyone
  • Accelerator and Physics Workshops in November

5
Tevatron Performance
Tevatron peak and integrated luminosities
6
2007 Accelerator Shutdown
  • Accelerator work appears to have gone well
  • Significant work on several of the machines
  • Experiments confined efforts to remedial work
  • Silicon Readout recoveries
  • CDF Silicon Cooling system
  • All Experimenters Meeting at 4 pm TODAY Curia
    II

7
Shutdown 2007
8
Shutdown 2007
9
Shutdown 2007
10
Vulnerability Review
  • Director commissioned a review of experiment
    vulnerability
  • What can we expect to break?
  • With what vulnerability?
  • What are appropriate remedial actions?
  • Committee
  • Chair Dan Green array of detector experts
  • Excellent Cooperation from the experiments
  • No Show stoppers
  • Need to work on preserving corporate knowledge
    and expertise

11
Neutrino Program
12
SciBooNE
13
MINOS Results
14
MiniBooNE Results
15
Future Neutrino Experiments
  • MINERvA
  • Neutrino Cross Sections
  • To be mounted in front of MINOS Near Detector
  • RD and construction preparation is well advanced
  • Has full completed all CD3 requirements, awaiting
    ESAAB (Nov. 1 ) and start of construction
  • NOvA
  • Long Baseline, Off Axis from NuMI
  • Enormous Far Detector
  • Lots of RD and design work complete
  • Successfully completed CD2 Baseline review
  • Construction start of Road in Minesota in Spring
    2008
  • BNL-FNAL Long Baseline Study

16
P5 Committee
  • Tevatron Running in 2009 June 2007
  • Concerned with
  • the continued good progress of integrated
    luminosity
  • The understanding of the collaboration manpower
  • The understanding of the Laboratory support for
    operations
  • Conclusion was clearly positive
  • Tevatron Running in 2010 September 2007
  • Wanted to see physics progress
  • Understand opportunity cost
  • Anticipated nothing new on effort front

17
Tevatron Luminosity Delivery for Run II
FY10 start
Real data for FY02-FY07
FY09 and FY10 integrated luminosities assumed to
be identical
FY08 start
18
Criteria for Tevatron Runningin FY 2010
  • Pier Oddone
  • September 24, 2007

19
Criteria for running in 2010
  • Important Physics
  • Viable Collaborations
  • Acceptable damage to other programs

20
Important Physics
  • We explore uniquely a large variety of physics at
    the energy frontier until LHC detectors overtake
    us
  • Sensitivity to 160 GeV Higgs at 95 CL, opens in
    the next year
  • Low mass Higgs (Standard or lowest lying MSSM
    Higgs below 150 GeV) is hard to reach early with
    the LHC

21
Road to Higgs and Beyond
?
Total Inelastic
BsBs Oscillation, ?b Discovery Precision Meas.
jets (qq, qg, gg)
mb -
-
-
bb
observed
?b -
MW 0.05
W Z
Mtop 1.2
nb -
-
tt
Observed WZ, Evidence for ZZ and Single Top
WZ, Single Top, ZZ
pb -
Higgs
WH,ZH
MHiggs lt ? GeV at 95 CL
Low Mass SUSY
fb -
-
-
-
100 120 140 160 180 200
Higgs Mass GeV/c2
22
SM Higgs Searches
23
Constraint MSSM (CMSSM)
With Electroweak precision measurements and cold
dark matter density (WMAP, )
Sven Heinemeyer, Georg Weiglein
24
W and Top Mass, and SM Higgs
Will Tevatrons prediction and observation/exclusi
on agree with what LHC sees?
25
SM Higgs Searches at Tevatron
26
Important Physics
  • From first collisions at the LHC in Summer 2008
    and closure of Tevatron September 2009 is too
    short for LHC detectors to wipe CDF/D0 out
  • Any delay in putting the hardware together no
    float now
  • Delay in first beam to collisions only three
    months now
  • Natural time to accumulate luminosity
  • Debugging detector and software
  • Physics analysis

27
Viable Collaborations
  • The collaborations should be viable through
    FY2009
  • To ensure collaborations are viable in FY2010, we
    need to start working now to make sure there are
    enough students/post-docs and know how
  • Early results from LHC could negatively impact
    the collaborations in 2010 if most folks were to
    decamp Should we be so lucky!!

28
Viable Collaborations
  • Conversely, if there are delays in getting
    results from LHC, the Tevatron remains exciting,
    producing physics for students/postdocs/faculty
  • In the middle, there could be a horse race to the
    Higgs
  • To keep collaborations viable need agency support
    of University groups for work at the Tevatron
    beyond 2010

29
Acceptable damage
  • Running in 2010 delays slightly 700kW neutrino
    beam capability
  • Running in 2010 has modest impact on NOvA
    start-up (presently shut-down starts late 2010
    physics run June 2011)
  • Requires additional resources not to slow down
    the ILC RD, Project X, or neutrino program
    approximately 30M

30
Conclusion
  • We believe strongly that DOE should plan to run
    through FY2010
  • An early recommendation by P5 would help the
    planning effort for the lab and collaborations.

31
Conclusions for IFC
  • 2007 has been a very active year for Fermilab on
    every front.
  • Accelerator and Detector Operations in 2007 were
    great
  • Physics Output from Tevatron Collider is
    phenomenal
  • Shutdown work was successfully accomplished
  • Accelerator Complex is starting up
  • With P5 we have
  • Recommendation for 2009 running
  • Proposed running Tevatron in 2010 decision in
    2008.
  • Looking forward to a productive 2007
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