Department of Energy Office of Science DOE Office

Department of Energy Office of Science DOE Office of High Energy Physics Report to the Astronomy and Astrophysics Advisory Committee Agency Overview Kathy Turner Office of High Energy Physics, Office of Science Department of Energy Oct. 14 th, 2008 1

Department of Energy Office of Science 2

Department of Energy Office of Science 3

Department of Energy HEP Organization Chart Office of High Energy Physics Dennis Kovar HEP Budget and Planning Dean Oyler *Jerry Blazey (IPA) HEP Operations Kathy Yarmas Marsha Marsden Katie Perine *Rachel Grayson Research & Technology Division Facilities Division Glen Crawford Dennis Kovar Sherry Pepper-Roby Donna Lang Kristi Naehr Physics Research Wanda Morris Proton Accelerator Technology Physics Accelerator Science Saul Gonzalez Phil Debenham Amber Boehnlein (Detailee) Dave Muller (IPA) Electron Accelerator Physics *John Kogut Non-Accelerator Physics *Kathy Turner Eli Rosenberg (IPA) Theoretical Physics Chung Leung (IPA) *Denotes base position Vera Bibbs Rachel Grayson Facility Operations Fermilab Complex Mike Procario Detector R&D Howard Nicholson (IPA) Computational HEP Amber Boehnlein (Detailee) John Kogut Don Petravick (Detailee) Other Operations (SLAC/Other Labs) John Kogut SBIR/STTR L. K. Len Office of Science LHC Operations Facilities Development General Accelerator R&D Bruce Strauss LARP *L. K. Len SRF R&D Bill Weng (IPA) ILC R&D Jerry Blazey (IPA) Instrumentation & Major Systems NOv. A – Mike Procario Minerva – Ted Lavine (IPA) Daya Bay – Ted Lavine (IPA) DES – Kathy Turner CDMS – Howard Nicholson (IPA) JDEM – Kathy Turner 4

Department of Energy Office of Science 5

Department of Energy The Office of Science Note: The FY 08 appropriation was $689 M. Later, we received $32 M as a supplement Total FY 08 = $721 M. Our FY 08 “base” remained at $689 M. Office of Science 6

SC Request vs. Appropriation History (FY 2008$) Department of Energy Office of Science 7

DOE Office of Science (SC) Department of Energy Office of Science § The Office of Science is the single largest supporter of basic research in the physical sciences in the United States, providing more than 40 percent of total funding for this vital area of national importance. It oversees – and is the principal federal funding agency of – the Nation’s research programs in high-energy physics, nuclear physics, and fusion energy sciences. § The Office of Science provides grants to universities and other institutions to work on research in our program. § The Office of Science manages 10 world-class laboratories, which often are called the “crown jewels” of our national research infrastructure. The national laboratory system, created over a half -century ago, is the most comprehensive research system of its kind in the world. Ø Five are multi-program facilities: Argonne National Laboratory, Brookhaven National Laboratory, Lawrence Berkeley National Laboratory, Oak Ridge National Laboratory, and Pacific Northwest National Laboratory. The other five are single-program national laboratories: Ames Laboratory, Fermi National Accelerator Laboratory, Thomas Jefferson National Accelerator Facility, Princeton Plasma Physics Laboratory, and Stanford Linear Accelerator Center. 8

DOE Office of Science (SC) Office of High Energy Physics (OHEP) Department of Energy Office of Science DOE OHEP Program is the U. S. Federal Steward of HEP research § providing over 90 % of federal support (remainder primarily NSF) Ø designs, constructs and operates research facilities Ø supports researchers at universities and laboratories to carry out the research Ø develops advanced technologies and next generation scientific/technical workforce OHEP’s Mission is to maintain the Nation’s competency/leadership in HEP research § With the responsibility to Ø establish a strategic plan that address the identified scientific opportunities Ø formulate, justify and defend Budget Requests to implement that plan Ø effectively manage the funding obtained to deliver significant outcomes 9

DOE Office of Science (SC) Office of High Energy Physics (OHEP) Department of Energy Office of Science 10