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Dark Energy Task Force. Background OSTP convened Interagency Working Group (NSF/NASA/DOE) on Physics of the Universe under NSTC OSTP convened Interagency.

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Presentation on theme: "Dark Energy Task Force. Background OSTP convened Interagency Working Group (NSF/NASA/DOE) on Physics of the Universe under NSTC OSTP convened Interagency."— Presentation transcript:

1 Dark Energy Task Force

2 Background OSTP convened Interagency Working Group (NSF/NASA/DOE) on Physics of the Universe under NSTC OSTP convened Interagency Working Group (NSF/NASA/DOE) on Physics of the Universe under NSTC IWG produced an integrated plan for Physics of the Universe IWG produced an integrated plan for Physics of the Universe Astronomy and Astrophysics Advisory Committee formed – expanded and reformulated by NSF Authorization (NSF/NASA/OSTP) Astronomy and Astrophysics Advisory Committee formed – expanded and reformulated by NSF Authorization (NSF/NASA/OSTP) AAAC will report to NASA/NSF/DOE/OSTP as of March 15, 2005; DETF will report to AAAC and HEPAP AAAC will report to NASA/NSF/DOE/OSTP as of March 15, 2005; DETF will report to AAAC and HEPAP

3 Physics of the Universe

4 Motivation The joint Dark Energy Task Force (DETF) will help the agencies to identify actions that will optimize a near- and intermediate-term dark energy program and ensure rapid progress in the development and implementation of a concerted effort towards understanding the nature of dark energy.

5 Elements of Charge 1. Summarize the existing program of funded projects by projected capabilities, systematics, risks, required developments and progress-to- date. 1. Summarize the existing program of funded projects by projected capabilities, systematics, risks, required developments and progress-to- date. 2. Where possible, similarly evaluate proposed and emergent approaches and techniques for dark energy studies; that is, characterize these approaches and techniques by the added value the projected capabilities would provide to the investigation of dark energy. 2. Where possible, similarly evaluate proposed and emergent approaches and techniques for dark energy studies; that is, characterize these approaches and techniques by the added value the projected capabilities would provide to the investigation of dark energy. 3. Identify important steps, precursors, R&D and other projects that are required in preparation for JDEM, LST and other existing or planned experiments. 3. Identify important steps, precursors, R&D and other projects that are required in preparation for JDEM, LST and other existing or planned experiments. 4. If possible, identify any areas of dark energy parameter space that the existing or proposed projects fail to address. 4. If possible, identify any areas of dark energy parameter space that the existing or proposed projects fail to address.

6 Guidance The DETF is not constituted, nor has available time, to review individual proposals to determine their technical feasibility or likelihood of meeting performance goals. Rather, in addressing the areas above the DETF is asked to advise on the coverage of parameter space, to identify potential knowledge gaps that would preclude informed decisions about projects, to identify unnecessary or duplicated efforts, and to quantify the sensitivity of the determination of dark energy parameters to experimental performance goals such as sky coverage, number of objects, image quality or other requirements. The DETF should also comment on areas where expanded theoretical or modeling activity would be of significant benefit. The DETF is not constituted, nor has available time, to review individual proposals to determine their technical feasibility or likelihood of meeting performance goals. Rather, in addressing the areas above the DETF is asked to advise on the coverage of parameter space, to identify potential knowledge gaps that would preclude informed decisions about projects, to identify unnecessary or duplicated efforts, and to quantify the sensitivity of the determination of dark energy parameters to experimental performance goals such as sky coverage, number of objects, image quality or other requirements. The DETF should also comment on areas where expanded theoretical or modeling activity would be of significant benefit.

7 Confirmed DETF Members Rocky Kolb, Chair Rocky Kolb, Chair Andy Albrecht Andy Albrecht Bob Cahn Bob Cahn Wendy Freedman Wendy Freedman Jackie Hewitt Jackie Hewitt Wayne Hu Wayne Hu Two more to come… John Huth Marc Kamionkowski Lloyd Knox Suzanne Staggs Nick Suntzeff


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