doe office of science office of high energy physics program update
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DOE Office of Science Office of High Energy Physics Program Update. Astronomy & Astrophysics Advisory Committee May 16, 2005. Kathy Turner. Kathy Turner, Feb. 7, 2005. Program News. - PowerPoint PPT PresentationTRANSCRIPT
Office of Science
U.S. Department of Energy
DOE Office of ScienceOffice of High Energy Physics
Program Update
Astronomy & Astrophysics Advisory CommitteeMay 16, 2005
Kathy Turner, Feb. 7, 2005Kathy Turner
Office of Science
U.S. Department of Energy
Program News
August 2004 -- International Committee for Future Accelerators (ICFA) endorsed International Technology Recommendation Panel’s report which recommended cold technology as the choice for the design of a new International Linear Collider
Moving forward on R&D for this technology; Barry Barish head of Global Design Effort
Subpanel on LHC/ILC – lay out science complementary science case
New National Academy study started 11/04:Elementary Particle Physics in the 21st Century - joint OHEP & NSF-EPP - OHEP and NSF jointly asked for and are funding the study
Dark Energy Task Force (DETF) formed - joint subpanel - reports to HEPAP & AAAC - Meetings 3/05 & 6/05
Task Force on CMB Research (TFCR) joint subpanel• final report coming soon
Joint Dark Energy Mission Science Definition Team (JDEM-SDT) formed• Meetings 11/04, 2/05, 6/05• Purpose: lay out the level 1 science requirements of a space-based dark energy mission &
provide advice to agencies
Office of Science
U.S. Department of Energy Office of ScienceFY 2006 Congressional
Budget Request
FY 2004
Comparable
Approp.
FY 2005
Comparable
Approp.
FY 2006
President’s
Request
FY 2006 Request vs FY 2005
Appropriation
Basic Energy Sciences 991,262 1,104,632 1,146,017 +41,385 +3.7%
Advanced Scientific Computing Res.
196,795 232,468 207,055 -25,413 -10.9%
Biological & Environmental Research
624,048 581,912 455,688 -126,224 -21.7%
High Energy Physics 716,170 736,444 713,933 -22,511 -3.1%
Nuclear Physics 379,792 404,778 370,741 -34,037 -8.4%
Fusion Energy Sciences 255,859 273,903 290,550 +16,647 +6.1%
Other 383,620 270,471 278,734 +8,263 +3.1
Total, Science 3,547,546 3,604,608 3,462,718 -141,890 -3.9%
(dollars in thousands)
Office of Science
U.S. Department of Energy
High Energy Physics Program
Goal: Ultimate Unification
All are partnerships with NSF and/or Foreign
Operating:CDF and DZero Fermilab Tevatron (protons) Top quark, Higgs, SUSY, extra
dimensions
MiniBooNE Fermilab Main Injector Neutrino mixing
BaBar SLAC B-factory (electrons) Matter-antimatter, b quark, CP violation
NUMI/MINOS Fermilab main injector Neutrino mixing (long baseline)
Participation in operating experiments:CLEO Cornell
Super-K, K2K, KamLAND Japan neutrino mixing, proton decay
Belle Japan b physics
ZEUS DESY, Germany deep inelastic scattering
Approved/Construction:ATLAS & CMS CERN LHC (protons) Higgs, SUSY, extra dimensions
Proposed or Possible Future:
Linear Collider International (electrons) Higgs, SUSY, extra dimensions
Neutrino-less double beta decay experiment Majorana neutrinos & neutrino mass
Reactor Neutrino and/or Long Baseline Neutrino experiment - neutrino mixing
Office of Science
U.S. Department of Energy
High Energy Physics Program Goal: Cosmic Connections
Operating: Sloan Digital Sky Survey (w/NSF, foreign) dark matter, dark
energy Supernova Cosmology Project, Nearby Supernova Factory dark energyCryogenic Dark Matter Search, CDMS-II (underground, w/NSF) dark matter
Approved/Construction:Large Area Telescope (LAT) – GLAST mission (w/NASA, foreign) gamma rays,
dark matter
*Pierre Auger – ground array in Argentina (w/NSF, foreign) high energy cosmic rays
AMS – Alpha Magnetic Spectrometer – ISS (w/NASA, foreign) cosmic antimatter
VERITAS – telescope in Arizona (w/NSF, Smithsonian) high energy gamma rays
Axion Dark Matter eXperiment (ADMX) – at LLNL axion dark matter search
R&D, Proposed or Possible Future:CMB technology
JDEM (SNAP R&D) dark energy
Ground telescopes/cameras dark energy/matter
* Partial operations at current time
Office of Science
U.S. Department of Energy
FY 2004/05/06 HEP Budget (B/A in Millions)
FY 2004 FY 2005 FY 2006 Req. Change 06-05
Proton Accelerator-based Physics
Research $ 76.4 $ 75.7 $ 75.4
Facilities (other than LHC) 241.9 263.6 251.6
LHC 48.8 32.5 7.4
LHC Support 15.6 29.4 52.6
Subtotal $ 382.6 $ 401.1 $ 387.1 -3.5%
Electron Accelerator-based Physics
Research $ 27.0 25.5 24.9
Facilities 117.9 118.4 108.0
Subtotal $ 145.0 $ 143.9 $ 132.8 -7.7%
Non-Accelerator-based Physics $ 47.3 $ 46.9 $ 38.6 -17.8%
Theoretical Physics $ 49.4 $ 49.0 $ 49.1 +0.2%
Advanced Technology R&D $ 96.8 $ 94.7 $ 106.3 +12.3%
Construction/NuMI $ 12.4 $ 0.8 $ 0.0
TOTAL HEP Budget $ 733.6 $ 736.4 $ 713.9 -3.1%
SBIR & STTR (included in Advanced Tech R&D) $ (17.5) $ (17.9) $ (18.2)
Office of Science
U.S. Department of Energy
Non-Accelerator Physics Funding ($k)
actual as of 8/04 as of 5/05 Pres.Req.
Project fy03 fy 04 fy05 fy06 CommentsVERITAS -- 1,600 2,050 1,149 complete in fy06Auger 1,230 1,000 -- -- complete in fy04AMS 1,500 -- -- -- complete in fy04CDMS 790 550 -- -- complete in fy04GLAST/LAT 8,501 7,900 11,421 -- complete in fy05
Scientific Research (operating budget)labs 16,384 19,713 21,434 17,120univ. 12,300 13,565 15,871 16,500
Axion-I, ADMX 350 850 835 850Milagro 125 75 70 70SNAP R&D 3,065 2,950 2,762 2,900 pre-conceptual R&D
TOTAL 44M 47M 54M 39M
Office of Science
U.S. Department of Energy
The DOE HEP program in FY 2006
Overall HEP budget and priorities in FY 2006:
Tevatron and B-factory will be fully supported – these are our two major operating facilities
LHC preparations will be fully supported A reasonable level of support has to be maintained for the core
research program in the universities and laboratories Investment for mid- and long term new initiatives will come
from redirection DOE will not proceed with the BTeV project at Fermilab
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U.S. Department of Energy
Sloan Digital Sky Survey
2.5 m Telescope
Mosaic Imaging Camera
640 Fiber Spectrograph
Telescope in New Mexico
Taking data since 1998 - continues
Oct 2004 - 3rd public data release Data for 141 million objects over 5282 square degrees
Jan. ’05 – baryon oscillation measurement
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U.S. Department of Energy
Cryogenic Dark Matter Search
Purpose: direct detection of Weakly Interacting Massive Particles (WIMPS)
Location - Soudan Mine in Minnesota
Data-taking: partial operations started in 2003, full operations with 5 towers started recently & will continue until mid-2006
Results – April 2005
…set the world's lowest exclusion limits on the WIMP cross section by a factor of 10 compared to other experiments, ruling out a significant range of neutralino supersymmetric models.
CDMS-II
Blue line – new results
Dotted Blue line – expected full results
Office of Science
U.S. Department of Energy
Pierre Auger – high energy cosmic ray detector array (w/NSF & foreign partners)
Partial operations have started – construction expected to be completed by early 2006.
Current status: 18 (out of 24) fluorescence telescopes operating 833 (out of 1600) surface Cherenkov detectors deployed, 758 operating
3000 km2 site in Argentina
As of Fall 2003, it became the largest air-shower detector in the world
Fluorescence telescopes
water Cherenkov surface detectors
Office of Science
U.S. Department of Energy
Very Energetic Radiation Imaging Telescope Array System - VERITAS
Study of sources of very high energy gamma-rays in range of 50 GeV-50 TeV -- study extreme acceleration mechanisms Location: Kitt Peak 4 telescope array started construction Oct. 2003 Operations start Oct. 2006 Prototype telescope built and tested successfully
Partnership of DOE & NSF with contributions from Smithsonian + foreign
All work at Kitt Peak was stopped at the end of April pending resolution of a legal action due to environmental/historical issues by the Tohono O’odham Indian Nation. NEPA & NHPA being redone. Fabrication is proceeding at Whipple & universities on schedule. Hopefully work can start again in early Fall.
Office of Science
U.S. Department of Energy
Gamma Ray Large Area Space Telescope (GLAST) Mission
Primary Instrument: Large Area Telescope (LAT)- Collaboration between NASA, DOE, France, Italy, Japan, Sweden – managed at SLAC.- Recently had to be rebaselined. DOE’s contribution was increased by $3M to $45M,
where it has been capped.- DOE’s remaining scope is now well-defined deliverable – electronics modules. - LAT scheduled to leave SLAC in early 2006 – to NRL for environmental testing
Measurement of high energy gamma rays from space - Energy and direction of gamma rays from 20 MeV to 300 GeV over wide field of view - launch in 2007
Office of Science
U.S. Department of Energy
AMS - Alpha Magnetic Spectrometerw/NASA + foreign partners
• search for dark matter, missing matter & antimatter on the International Space Station
• Prototype (AMS-01) took data on STS-91 in 1998
• AMS-02 fabrication complete in 2005
• Launch and deployment on ISS currently planned for 2008.
Office of Science
U.S. Department of Energy
Dark Energy – Planning & Future
Developed DOE/NASA Joint Dark Energy Mission (JDEM) plan for a joint space-based mission – plan released 11/03 Science Definition Team formed; meetings 11/04 and 2/05
Purpose: lay out the level 1 science requirements of a space-based dark energy mission
JDEM is a high priority (tie for 3rd place) in DOE’s Facilities for the Future of Science 20 Year Plan JDEM & Large Survey Telescope (LST) are highest priority in the Interagency Physics of the Universe
report
Current Work: Supernova Cosmology Project (SCP) – continuing ground and HST measurements to collect
statistics over large redshift range Nearby Supernova Factory (SNFactory) – large sample of nearby supernovae to study
properties in detail
R&D efforts & planning Continuing R&D activities for SNAP — a concept for JDEM, using supernovae Dark Energy Survey (DES) – new camera for Blanco 4m telescope at CTIO - using galaxy cluster counting &
spatial clustering of galaxies – scientists are investigating participation Large Synoptic Survey Telescope (LSST) – using weak lensing - scientists are investigating participation
Office of Science
U.S. Department of Energy
DOE HEP Future Planning
In order to inform the Department of OHEP’s intent to pursue several new scientific
topics, we are preparing draft portfolio of medium-sized mid-term experiments
- Have compelling scientific case for:
Neutrino experiments such as: reactor-based neutrino experiment to measure θ13
Electron-neutrino appearance experiment - accelerator-based, to measure θ13 & resolve mass hierarchy
neutrino-less double beta decay experiment to probe the Majorana nature of neutrinos
Astrophysics: Underground experiment to search for direct evidence of dark matter Ground-based dark energy experiment
HEPAP subpanels will recommend which proposals to pursue.
Office of Science
U.S. Department of Energy
FY 2005 Funding Allocation
Accelerator based physics (proton & electron) ~74% Non-Accelerator physics ~6%
Theory ~6% Technology R&D ~13%
Theory
Tech R&D
Proton PhysicsElectron
Physics
Non-Accel Physics
$401M
$144M
$95M$49M$47M