LBNF/DUNE Update Public Meeting Sanford Lab Update

Slides:



Advertisements
Similar presentations
Dark Universe: Dark Matter, Dark Energy and the Fate of the Universe.
Advertisements

DOE Neutrino Program Plans
LBNE - PMT production testing workshop Xinhua Bai, SDSMT Peggy Norris, Sanford Lab & BHSU Tuesday, February 23, Madison, WI.
Dark Matter Searches with Dual-Phase Noble Liquid Detectors Imperial HEP 1st Year Talks ‒ Evidence and Motivation ‒ Dual-phase Noble Liquid Detectors ‒
Sept. 18, 2008SLUO 2008 Annual Meeting Vision for SLAC Science Persis S. Drell Director SLAC.
Neutron background measurement at LNGS: present status Measurement carried out in collaboration between LNGS ILIAS-JRA1 and ICARUS groups.
Peggy Norris, Black Hills State Univ/Sanford Underground Laboratory at Homestake.
PANDAX Results and Outlook
Search for Dark Matter at CJPL with PANDAX
Long-Baseline Neutrino Experiment James Strait LBNE Project Director Public Information Meeting May 23, 2013 LBNE-doc-7321.
International collaboration in high energy physics experiments  All large high energy physics experiments today are strongly international.  A necessary.
LBNE - PMT production testing workshop Tuesday, February 23, Madison, WI Xinhua Bai, SDSMT Robert McTaggart, SDSU Peggy Norris, Sanford Lab & BHSU.
Manuel Calderón de la Barca Sánchez Professor of Physics September 17, 2013, Videoconference at ITESM for IFI students Physics Department Opportunities.
NuMI NuMI Overview NBI 2002 S. Childress (FNAL) 14 March ‘02 NuMI / MINOS Overview.
Carter Hall, University of Maryland August 7, 2015 DPF 2015, Ann Arbor, MI The LZ WIMP dark matter search.
LSST CD-1 Review SLAC, Menlo Park, CA November 1 - 3, 2011 The Funding Agency Context for the LSST DESC Steve Kahn.
Recommendations for Science at SNOLAB Andrew Hime On behalf of the Experiment Advisory Committee Aug. 17, 2005 SNOLAB Surface Building.
The NSCL is funded in part by the National Science Foundation and Michigan State University. Determining the Impact Parameter and Cross-Section in Heavy.
LSC – Hanford 16 th - 19 th August 2004 The View from NSF Changes in NSF leadership Funding Interagency Working Group response to Q2C Outreach - New $5M.
Office of Science U.S. Department of Energy RHIC Users Meeting BNL; June 8, 2006 Gulshan Rai RHIC/AGS Users Meeting Gulshan Rai Program Manager for Heavy.
Dark Matter Detection with Liquid Xenon Masahiro Morii Harvard University Laboratory for Particle Physics and Cosmology 21 August
Long-Baseline Neutrino Facility LBNF LBNF/DUNE Logistics Workshop Summary Mike Headley August 19, 2015.
Cost and Engineering Working Group Introduction Jim Strait Fermilab LBNE Project Manager Deputy Chair, Cost and Engineering Working Group LBNE Reconfiguration.
Fermilab Neutrino Program Jim Strait Neutrino Discussion at CERN 26 November 2013.
A multi-stage liquid Xe based Dark Matter experiment at China JinPing Lab (location: Sichuan Province) Deepest dark matter facility, covered with 2,500m.
I NSTITUTE FOR S TRUCTURE AND N UCLEAR A STROPHYSICS N UCLEAR S CIENCE L ABORATORY CASPAR An underground Accelerator Laboratory for Nuclear Astrophysics.
May 6, 2006Henderson Dusel Capstone Meeting Low Background Counting A Facility Wish List for the New Underground Laboratory F. Calaprice.
A Brief Introduction to Quarknet and Particle Physics Mike Strauss.
DARK MATTER IN THE UNIVERSE? PRESENTED BY L. KULL AT THE R.H.FLEET SCIENCE CENTER December 14,2005.
Department of Energy Office of Science  FY 2007 Request for Office of Science is 14% above FY 2006 Appropriation  FY 2007 Request for HEP is 8% above.
Plan to go forward Peter Wilson SBN Program Coordinator 27 September 2014.
John Womersley 1/13 Fermilab’s Future John Womersley Fermilab May 2004.
DARK MATTER SEARCH Carter Hall, University of Maryland.
Neutrino Pre-Town Meeting This is a town meeting: make your voice heard!
Long-Baseline Neutrino Facility LBNF LBNF/DUNE Project 29 September 2015.
Detector R&D through the NSF PHY division. Jim Shank/Jim Whitmore, NSF CPAD Meeting Arlington, TX 5-7 October, 2015.
News from LBNF C. J. Mossey, LBNF Project Director DUNE Collaboration Meeting - South Dakota School of Mines and Technology 19 May 2016.
Long-Baseline Neutrino Facility LBNF Far Site Conventional Facilities (FSCF) Scope and Interface Overview Tracy Lundin as borrowed from Headley & Willhite.
Long-Baseline Neutrino Facility LBNF LBNF/DUNE Status N. S. Lockyer
Nigel Lockyer Fermilab Operations Review 16 th -18 th May 2016 Fermilab in the Context of the DOE Mission.
Long-Baseline Neutrino Facility LBNF LBNF Project C. J. Mossey, LBNF Project Director 49 th Annual Fermilab Users Meeting 16 June 2016.
Long-Baseline Neutrino Facility LBNF LBNC: Far Site Update and Planning Mike Headley LBNF Far Site Facilities Project Manager January 11, 2016.
Challenges to get LBNF ready for Far Detector installation ASAP Elaine McCluskey ELBNF Proto-Collaboration Meeting 22 Jan 2015.
“Megaton” Cerenkov Detector - Excavation Kenneth Lande, Univ. of Pennsylvania 4200 mwe Depth.
Long-Baseline Neutrino Experiment James Strait LBNE Project Director Public Information Meetings June 25-26, 2013 LBNE-doc-7321.
THE SOUTH DAKOTA DAVIS- BAHCALL SCHOLARS PROGRAM Peggy Norris Deputy Director of Education and Outreach
Long-Baseline Neutrino Facility LBNF Elaine McCluskey, LBNF Project Manager Fermilab PAC Meeting 23 June 2015.
Muon Ionisation Cooling Experiment Overview
LIGO Educational Outreach: The Science Education Center
FOUNDATION BOARD MEETING
Overview of the Long-Baseline Neutrino Facility Cryogenic System
PandaX DM Search Exp Xiangdong Ji (季向东)
Jefferson Lab Overview
A Brief Introduction to Quarknet and Particle Physics
Risk Identification HL-LHC Detector Upgrades Project
General Issues We will need to understand infrastructure requirements
QuarkNet and Cosmic Ray Muon Flux Experiments
Laboratory for Underground Nuclear Astrophysics
George’s Brigade.
Welcome! APPEAL-2 Accelerator and Particle Physics Education at A-Level Particle Accelerators - Shedding Light on the Dark Universe July 2, 2011 University.
University of South Dakota
SuperCDMS at SNOLAB Wolfgang Rau Queen’s University for the
Harry Nelson UCSB DUSEL Henderson at Stony Brook May 5, 2006
HCS Elementary Education Department
Yet Another Report from DOE Office of High Energy Physics
UCLA High Energy & Astro-Particle (HEAP) Seminar
Starting Points (Collaboration ; Laboratory ; Magnetic Moment Results)
Facilities Initiative Chris Kinsley, Director, Finance & Facilities
Office of Research & Commercialization
The Estimated Limits For A 5g LE-Ge Detector
Presentation transcript:

LBNF/DUNE Update Public Meeting Sanford Lab Update Mike Headley SDSTA Executive Director and Sanford Lab Director 13 March 2017

Sanford Underground Research Facility Dedicated facility for underground scientific research Open Cut Yates Complex Visitor Center Created by the State of South Dakota with major philanthropic donations from Barrick (property) and T. Denny Sanford ($70M). Continued support by the State of South Dakota ($46M through 2016). Operations funded by US Dept of Energy, through a subcontract between Fermilab and the SDSTA. Ross Complex 186 acres (surface) 7700 acres (underground)

4850L Science Facilities Existing Facilities Future Facilities M. Headley | Sanford Lab Update

Current Underground Science Program Physics (4850L Davis Campus) Majorana Demonstrator: Studying the neutrino’s mass and the matter/antimatter imbalance in the universe. Proving techniques for a larger experiment. Status: 2 cryostats with 44 detectors (40kg Ge) assembled. Commissioning and testing underway. Physics data in mid-2017. - overview of the current Sanford Lab science program Large Underground Xenon (LUX): Direct detection of dark matter. Status: Data taking completed in May 2016. Remains most sensitive DM experiment in world. Decommissioning underway in prep for the LUX-ZEPLIN (LZ) next generation experiment. M. Headley | Sanford Lab Update

Current Underground Science Program Physics (4850L Ross Campus) Compact Accelerator System for Performing Astrophysical Research (CASPAR): Studying nuclear reactions in stars resulting in the generation of elements heavier than Iron. Status: SDSM&T faculty and students leading onsite activities. Beamline components assembled, commissioning underway. Operations planned mid-2017. Black Hills State University (BHSU) Underground Campus: Low background counting to characterize radiopurity of detector components. Status: Installed 4 low background counters. Completed counting activities for the first 45 LZ photo multiplier tubes. Providing opportunities for undergraduate students. - overview of the current Sanford Lab science program M. Headley | Sanford Lab Update

LUX-ZEPLIN (LZ) Dark Matter Experiment LZ will be located in the Davis Cavern on the 4850 foot level LZ collaboration includes ~220 members at 36 institutions. 10,000 kg Xe (3,500 gallons). 30x larger, 100x more sensitive than LUX. Using existing Surface Laboratory and 4850L Davis Campus facilities. Experiment and facility design work underway. Project has been “baselined” for construction. Facility modifications are underway on the surface and are planned for 2018 underground in Davis Campus. Experiment installation underground planned for 2018-19. Operate for 5 years starting ~2020. - Compared to initial sensitivities for direct-search detectors in 1980s, LZ represents improvement of 10^8 or 100M! (10^-48 vs 10^-40 cm2) LZ Detector and Shielding M. Headley | Sanford Lab Update

LZ Surface Construction Surface facility construction to complete in May 2017 M. Headley | Sanford Lab Update

Ross Shaft Refurbishment Update 4,679 feet down from surface (90% complete overall) Ross Shaft constructed in 1930s. Rehabilitation initiated in August 2012 to modernize the shaft for LBNF construction. SDSTA self-performing the project. Includes removal of old shaft steel and installation of ~6M pounds of new steel. Set to finish Q4 CY2017. Project total cost $32.2M: $5.95 in SD appropriated funds, $11.6M in U.S. DOE federal funds, and $14.6M in Sanford private funds. Surface Tramway   300 L 800 L 1250 L 1400 L 1550 L 1700 L 1850 L 2000 L 2150 L 2300 L 2450 L 2600 L 2750 L 2900 L 3050 L 3200 L 3350 L 3500 L 3650 L 3800 L 3950 L 4100 L 4250 L 4400 L 4550 L 4700 L 4850 L 5000 L Schedule Q1 CY2014 Completed Q1 CY2015 Q1 CY2016 Q1 CY2017 Q4 CY2017

Sanford Lab Educational Opportunities for K-12 Students Elementary A Day in the Life… Particle Accelerators Middle School Career Opportunities Dark Matter High School Neutrinos Elementary Exploring Unseen Force Be With You Middle School Seismic Science Search Dark Matter High School Perplexing Puddles Star-Stuff In Development There & Back Again Waterworks Opportunities to visit the lab are limited. School visits available: Fall Spring School Presentations Curriculum Units Field Trips M. Headley | Sanford Lab Update

Sanford Lab Education and Outreach Impacts K-12 students served from September 2015 to February 2017   School Presentations Curriculum Units Field Trips Number of Students 14,064 2,231 944 Number of Classrooms 1004 159 67 Before 2015, Sanford Lab’s E&O Program focused primarily on field trips. The total number of K-12 students participating in programming from 2008 to the end of February 2017 is 23,352. M. Headley | Sanford Lab Update

Sanford Lab Education and Outreach Activities in South Dakota Not represented Alliance, NE Upton, WY School Presentations Curriculum Units Field Trips M. Headley | Sanford Lab Update

Economic Impacts in South Dakota Through Year End CY2016 Spending in South Dakota to date $171M Annual total budget (all sources & activities) $23.4M Annual SURF operations budget (DOE funds) $14.75M Annual payroll in SD $13.6M Annual non-payroll expenses in SD $5.9M Jobs in South Dakota 163 Active research groups 24 Research groups with SD members 18 M. Headley | Sanford Lab Update

Total Spending in South Dakota through year end 2016 Grouped by 3-digit zip code region.

Full report available at: http://lbnf.fnal.gov/economic-impact.html M. Headley | Sanford Lab Update