the doe high energy physics program
Download
Skip this Video
Download Presentation
The DOE High Energy Physics Program

Loading in 2 Seconds...

play fullscreen
1 / 19

The DOE High Energy Physics Program - PowerPoint PPT Presentation


  • 80 Views
  • Uploaded on

The DOE High Energy Physics Program . Kathy Turner Office of High Energy Physics DOE Office of Science Fundamental Physics in Space Conference Warrenton, VA May 24, 2006. DOE Office of High Energy Physics (HEP). Goal is to Explore the Fundamental Interactions of Energy, Matter, Time,

loader
I am the owner, or an agent authorized to act on behalf of the owner, of the copyrighted work described.
capcha
Download Presentation

PowerPoint Slideshow about 'The DOE High Energy Physics Program' - nia


An Image/Link below is provided (as is) to download presentation

Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author.While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server.


- - - - - - - - - - - - - - - - - - - - - - - - - - E N D - - - - - - - - - - - - - - - - - - - - - - - - - -
Presentation Transcript
the doe high energy physics program

The DOE High Energy Physics Program

Kathy Turner

Office of High Energy Physics

DOE Office of Science

Fundamental Physics in Space Conference

Warrenton, VA

May 24, 2006

doe office of high energy physics hep
DOE Office of High Energy Physics (HEP)

Goal is to Explore the Fundamental Interactions of Energy, Matter, Time,

and Space

  • Understand the unification of fundamental particles and forces and the mysterious forms of unseen energy and matter that dominate the universe
  • Search for possible new dimensions of space

 Connections between the physics of

elementary particles and the physics that

determines the structure of the universe

HEP Office supports ~ 90% of U.S. High

Energy Physics and coordinates with NSF,

NASA and international efforts

We coordinate our program with the

National Science Foundation (NSF),

NASA and International Efforts

Kathy Turner, 24May2006

slide3

Office of High Energy Physics (HEP)- Components of the Program

Accelerator-based physics is our primary tool 

  • Top quarks, Higgs search, extra dimensions, supersymmetry; neutrino studies, b-quarks, CP violation

Operating experiments: Accelerator Physics

CDF and DZero Fermilab Tevatron Top quark, Higgs, SUSY, extra dimensions

MiniBooNE Fermilab Main Injector Neutrino mixing

BaBar SLAC B-factory Matter-antimatter, b quark, CP violation

K2K Japan Neutrino mixing

MINOS Fermilab Main Injector Neutrino mixing (long baseline)

BES China (IHEP) charm and bottom quarks

Under Construction:

ATLAS & CMS CERN Large Hadron Collider Higgs, SUSY, extra dimensions

Proposed or Future Planning:

  • International Linear Collider Higgs, SUSY, extra dimensions
  • Electron Neutrino Appearance Experiment Neutrino mass, mixing, hierarchy
  • High Intensity Neutrino Beam Neutrino mass, mixing, hierarchy
today s tools currently running u s hep accelerator experiments
Today’s Tools:Currently Running U.S. HEP Accelerator Experiments

Tevatron at Fermilab

Neutrinos @ MINOS

B-factory at SLAC

Kathy Turner, 24May2006

slide6

Office of High Energy Physics (HEP)- Components of the Program

  • Non-accelerator physics – a growing and important sector 
  • Atmospheric, solar and reactor Neutrinos, dark matter, dark energy,
  • high energy cosmic & gamma rays

Operating experiments Physics

Super-K, KamLAND in JapanProton decay, neutrino mixing

Sloan Digital Sky Survey 3D sky map, dark energy

Supernova Cosmology Project, Nearby Supernova Factory dark energy

Cryogenic Dark Matter Search (CDMS) dark matter in cosmic rays

Approved & Under Construction:

Large Area Telescope (LAT) – on NASA GLAST mission gamma rays, dark matter

Pierre Auger – ground array in Argentina high energy cosmic rays

AMS – Alpha Magnetic Spectrometer – on ISS cosmic antimatter

VERITAS – telescope in Arizona high energy gamma rays

Axion Dark Matter eXperiment (ADMX) dark matter search

Proposed (far from an exhaustive list):

Reactor Neutrino Experiment – Daya Bay Neutrino mixing

Joint Dark Energy Mission (JDEM) – space based dark energy

Large-aperture Survey Telescope (LST) – ground-based dark energy

    • Dark Energy Survey Telescope (DES) – ground-based dark energy
    • Enriched Xenon Observatory (EXO) Majorana neutrino mass
slide7

Office of High Energy Physics (HEP)

Other Components of the Program are:

  • Theory – elementary particles and fields
  • Technology R&D - for accelerator and detector technologies

Plans for FY 2007- President’s Budget Request is ~8% increase

    • Fully support our operating facilities: Tevatron at Fermilab and B-factory at Stanford Linear Accelerator Center (SLAC)
    • Increased support for Large Hadron Collider experiments as construction completes & for our research program
    • R&D for new initiatives

Kathy Turner, 24May2006

the scientific context discovery
The Scientific Context - Discovery

Plans for FY 2007  R&D Investment in Future Initiatives:

      • International Linear Collider
      • new neutrino experiments – accelerator & reactor
      • long-term accelerator technologies
      • Dark Energy - Increase R&D for ground- and space-based concepts
  • We are entering the age of the Terascale energies
    • The reigning theory (Standard Model) is as precise as it is incomplete.
    • How the weak and electromagnetic forces unify is a mystery …but the consequences are likely dramatic
  • Dark Energy & Dark Matter (what the … is it?)
  • Neutrinos – what are they and how do they interact?

Kathy Turner, 24May2006

advisory panels
Advisory Panels

High Energy Physics Advisory Panel (HEPAP) – reports to DOE and NSF

  • Expanded to 20 members, with members from Europe and Asia

AAAC – reports to DOE, NASA, NSF

Panels Reports to Topic(s) ReportsDue/Approved

CMB Task Force HEPAP & AAAC Roadmap future initiatives Oct 2005

P5 HEPAP B-factory + Tevatron Ops Nov 2005

Roadmap New mid-scale initiatives End 2006

NuSAG HEPAP & NSAC Double Beta Decay Exp’ts Sept 2005 Reactor and off-axis expt’s Feb 2006

Super neutrino beam Feb 2007

HEP Resources HEPAP Are there enough physicists Jan 2006

to run the program?

ILC & LHC HEPAP ILC/LHC “synergy” Mar 2006

Dark Energy HEPAP & AAAC Dark Energy techniques May 2006

Task Force

AARD HEPAP US Accel R&D program July 2006

Dark Matter SAG HEPAP & AAAC Direct Dark Matter experiments Feb 2007

Kathy Turner, 24May2006

national academies panel elementary particle physics in the 21 st center epp2010
National Academies Panel Elementary Particle Physics in the 21st Center (EPP2010)
  • A new “decadal survey”
    • Lay out the grand questions that are driving our field
    • Describe the opportunities that are ripe for discovery
    • Identify the tools that are necessary to achieve the scientific goals
    • Articulate the connections to other sciences and to society
    • Foster emerging worldwide collaboration
    • Recommend a 15 year implementation plan with realistic, ordered priorities
  • Not a typical high energy physics advisory panel. It includes
    • Non-physicists
      • Strengthen connections with society
      • Sharpen the physics questions
    • Non-particle physicists
      • Engage other scientific communities
    • International participants
      • Place US HEP in the international setting

Kathy Turner, 24May2006

nrc panel elementary particle physics in the 21 st center epp2010
NRC PanelElementary Particle Physics in the 21st Center (EPP2010)

Committee Chair: Harold T. Shapiro, president emeritus and professor of economics and public affairs, Princeton

Draft report release on 4/28/06 – www.nationalacademies.org/bpa/epp2010.html

Recommendations in priority order:

  • Fully exploit the opportunities for U.S. involvement at the Large Hadron Collider (LHC) at CERN
  • Comprehensive program to become the world-leading center for R&D for the International Linear Collider (ILC) and mount a compelling to build it in the U.S.
  • Expand the program in particle astrophysics and pursue an internationally coordinated, staged program in neutrino physics.

Kathy Turner, 24May2006

Now will show some of our astrophysics and cosmology related efforts & projects 

dark energy planning future
Dark Energy – Planning & Future

 Investigating future space and/or ground telescopes in cooperation with NASA and NSF.

 Dark Energy Projects are being considered by P5 panel.

 Planning how to review and select which project(s) go forward – in view of DETF report

  • Continue to plan a Joint Dark Energy Mission with NASA & we’re open to the possibility of International Collaboration
    • High priority in DOE Strategic Plan
    • DOE/NASA Science Definition Team

Dark Energy R&D:

Doing R&D for SuperNova Acceleration Probe (SNAP) concept for JDEM

Labs doing small amount of R&D for DES (Dark Energy Survey) and LSST (Large-scale Synoptic Survey Telescope)

In FY07 Request, additional R&D of ~$5M available – ground and/or space concepts will be selected by open competition; DETF will guide us

        • funding levels reflect tentative plan which may change based upon advice from DETF and other relevant considerations

Taking Data:

  • Nearby Supernova Factory – continues operations; measurements of nearby supernovae
  • Supernova Cosmology Project
    • Operations continuing using ground telescopes & Hubble measurements to collect statistics and refine results
  • Sloan Digital Sky Survey

Kathy Turner, 24May2006

office of high energy physics program sloan digital sky survey sdss
Office of High Energy Physics ProgramSloan Digital Sky Survey (SDSS)

Data

- Galaxy surveys, dark matter, dark energy

- June 2005 – 4th public data release

Taking data since 1998

- Approved for additional data-taking thru summer 2008

Funding: Sloan Foundation, NSF, DOE, Japan, Germany

Science News: Jan. 2005 – first baryon oscillation measurement

Mosaic Imaging Camera

Kathy Turner, 24May2006

Telescope in New Mexico

640 fiber spectrograph

slide14

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 starting soon & will continue in FY07

CDMS detector

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.

Also have Axion Dark Matter Search (ADMX) experiment at Lawrence Livermore Lab in California – another possible form of Dark Matter

Blue line – new results

Dotted Blue line – expected full results

Kathy Turner, 24May2006

pierre auger high energy cosmic ray detector array w nsf foreign partners
Pierre Auger – high energy cosmic ray detector array (w/NSF & foreign partners)

Water Cherenkov surface detectors

  • Search for Very High Energy cosmic rays
  • 3000 km2 site in Argentina
  • As of Fall 2003, it became the largest air-shower detector in the world

Fluorescence telescopes

Partial operations have started – construction expected to be completed by early 2007

 First science results out in Summer 2005 - a new cosmic ray spectrum at the highest energies; the results of anisotropy and point source searches; and new limits on the photon content of the primaries

Current status (April 2006)

- 18 (out of 24) fluorescence telescopes operating; rest under construction

- 1128 (out of 1600) surface Cherenkov detectors deployed, ~ 1000 operating

Kathy Turner, 24May2006

veritas very energetic radiation imaging telescope array system
VERITAS(Very Energetic Radiation Imaging Telescope Array System)
  • Scientific Purpose: Study of celestial sources of very high energy gamma-ray sources in the energy range of 100 GeV- 50 TeV & search for dark matter candidates
    • Atmospheric Cherenkov 4 12m telescope array w/500 pixel cameras
    • Energy range 100 GeV – 50 TeV
    • Angular resolution ~ 4’
    • Crab rate ~ 50 photons/minute
  • Funding: NSF, DOE + contributions from Smithsonian & foreign institutions

Status: Plan is to build at Kitt Peak.

  • In April 2005, work at Kitt Peak was stopped to redo the NEPA and NHPA process could be redone according to specifications
    • NSF is leading the process with DOE cooperating.
    • Had “government to government” meeting with Tohono O’odham Nation in January 2006
    • Plan is to install and commission the telescopes at the Whipple Basecamp while waiting for Kitt Peak access. A 2-year engineering run will start in 2007.

Two telescope array at Whipple Basecamp

Artist’s conception – 4 telescope array

Kathy Turner, 24May2006

glast large area telescope lat
GLAST Large Area Telescope (LAT)
  • GLAST will have a very broad science menu that includes:
  • Systems with supermassive black holes (Active Galactic Nuclei)
  • Gamma-ray bursts (GRBs)
  • Pulsars
  • Solar physics
  • Origin of Cosmic Rays
  • Probing the era of galaxy formation, optical-UV background light
  • Solving the mystery of the high-energy unidentified sources
  • Discovery! Particle Dark Matter? Other relics from the Big Bang? Extra dimensions? Testing Lorentz invariance. New source classes.
  • LAT is the primary instrument on NASA’s Gamma-ray Large Area Space Telescope (GLAST) mission
  • -- Collaboration between NASA, DOE, France, Italy, Japan, Sweden & managed at SLAC.
  • Shipped from SLAC to NRL for environmental testing in mid-May
  • GLAST launch scheduled for September, 2007
  • Successful DOE/NASA partnership!

GLAST draws the interest of both the the High Energy Particle Physics and High Energy Astrophysics communities.

GLAST is the highest-ranked initiative in its category in the National Academy of Sciences 2000 Decadal Survey Report.

Kathy Turner, 24May2006

ams alpha magnetic spectrometer w nasa foreign partners

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; integration and test to be completed in 2007
  • Plan is for a Shuttle Launch and deployment on ISS -- launch date is currently unknown.
high energy physics program
High Energy Physics Program

In years to come, we are looking forward to exciting

new discoveries at the TeV scale, with neutrinos and in

finding out what the stuff is that the majority of the

universe is made of – dark matter, dark energy

Kathy Turner, 24May2006

ad