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APS Neutrino Study: Reactor Working Group

APS Neutrino Study: Reactor Working Group. Goals of Working group:. Clear statement of physics potential of reactor experiments including non-  1 topics Understand physics reach, cost, and timescale for different scenarios Small (CHOOZ-2): fixed 10-ton detectors at 1.1 km baseline

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APS Neutrino Study: Reactor Working Group

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  1. APS Neutrino Study: Reactor Working Group Goals of Working group: • Clear statement of physics potential of reactor experiments including non-1 topics • Understand physics reach, cost, and timescale for different scenarios • Small (CHOOZ-2): fixed 10-ton detectors at 1.1 km baseline • Medium: 50-ton detectors (Movable vs Fixed) • Large: 250-1000 ton (single or multiple far detectors) • For each scenario, describe defensible strategy for reaching the • claimed systematic uncertainty. (What will be needed to establish a signal?) • How do these scenarios complement and compete with other reactor • and accelerator experiments around the world? APS Neutrino Study

  2. Saturday Agenda 1:30 – 3 Intro Ed Brief review of sites: Kashiwazaki Suekane (Ed) (10) Brazil Dave (10) Daya Bay Kam-Biu (15) Braidwood Jon (10) Diablo Canyon Karsten (10) 3-3:30 Coffee 3:30 – 5:30 Non-theta13 physics Beyond theta13 Gabriela (30) Neutrino magnetic moments, etc. Rabi (30) sin2W Janet (30) “Finese” Jon (10)

  3. Sunday Agenda 8:30 Breakfast 9:00 – 12:30 Double-Chooz Thierry, Hervé Sensitivity studies Mike Figures of merit for site comparison Karsten, Jon Importance of energy spectrum fits Dave Calibration strategies Josh 12:30 Lunch Discussion / Plans

  4. Meeting Plans • Phone / video meeting in early April (immediately after “mid-course correction” • meeting of working group leaders, study organizers) • Two-day meeting on west coast in mid-May. • Final general meeting of full APS study in late June.

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