US Funding Situation Three second generator (G2) dark matter experiments selected by DOE, NSF (and P5) summer 2014 http://www.symmetrymagazine.org/article/july-2014/us-reveals-its-next-generation-of-dark-matter-experiments.

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Presentation transcript:

US Funding Situation Three second generator (G2) dark matter experiments selected by DOE, NSF (and P5) summer 2014 http://www.symmetrymagazine.org/article/july-2014/us-reveals-its-next-generation-of-dark-matter-experiments http://science.energy.gov/hep/community-resources/next-generation-of-direct-detection/ LZ, SuperCDM-SNOLAB, ADMX-Gen2 CYGNUS 2015 Sven Vahsen (U. Hawaii)

US Funding Outlook CYGNUS 2015 Sven Vahsen (U. Hawaii)

US Funding Outlook CYGNUS 2015 Sven Vahsen (U. Hawaii)

US Funding Outlook CYGNUS 2015 Sven Vahsen (U. Hawaii)

US Funding Outlook CYGNUS 2015 Sven Vahsen (U. Hawaii)

US types of proposals US Department Of Energy (DOE) HEP University grants: Cosmic / intensity / energy / R&D “projects”: go through a DOE critical decision process. Funding separate from university grants, overseen by national labs. National Science Foundation (NSF) Individual proposal collaborative proposal CYGNUS 2015 Sven Vahsen (U. Hawaii)

Plan Engage DOE for R&D funds this fall Pixel readout plane + pixel chip design with LBNL Coherent neutrino scattering w/ COHERENT experiment Complete demonstration of SF6 TPC Submit NSF + DOE proposals summer 2017 Would like to have by then: a real CYGNUS collaboration White paper CYGNUS 2015 Sven Vahsen (U. Hawaii)