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Topics in Astroparticle and Underground Physics 2019/09/09 SNOLAB Update Jeter Hall Director of Research The SNOLAB Facility Hosted at the Vale Creighton Nickel Mine in Sudbury, Ontario, Canada Operated as a joint venture of 5 Canadian


  1. Topics in Astroparticle and Underground Physics 2019/09/09 SNOLAB Update Jeter Hall Director of Research

  2. The SNOLAB Facility • Hosted at the Vale Creighton Nickel Mine in Sudbury, Ontario, Canada • Operated as a joint venture of 5 Canadian Universities: Carleton, Queen’s, Montreal, Alberta, and Laurentian • Operations funded by the Canada Foundation for Innovation and the Province of Ontario • ~100 staff and >850 users from 128 institutions in 22 countries. 2

  3. Science at SNOLAB The science at SNOLAB is currently focused on fundamental particle physics. Primarily looking at further investigating the nature of matter . Specifically: • What is the nature of dark matter? • What is the nature of the neutrino? SNOLAB is interested in collaborating on any scientific research that benefits from deep underground facilities. For example: • Neutrino observatories (solar, supernovae, etc.) • Effects of radiation on biological systems • Environmental monitoring (nuclear non-proliferation, aquifers, 4D Earth, etc.) 3

  4. A A di dive verse se se set t of ex exper periment ental al pr projec ects s is is h hosted in in t the un undergr groun ound ca campus us 4

  5. Excellent progress from the current suite of experiments SNO+ is analyzing and publishing DEAP is analyzing and publishing CUTE has seen ionizing radiation PICO-40 has seen ionizing radiation DAMIC is analyzing and publishing HALO is analyzing, publishing, and ready REPAIR is growing 5

  6. data from SNOLAB @ TAUP C. Krauss talk from DM1 for PICO-40 update • T. Noble talk from DM10 for PICO future program • S. Westerdale and M. Boulay talks for DEAP-3600 analysis and results • • Also see many talks from other global argon efforts T. Aramaki in DM7 for SuperCDMS updates and status • A. Chavarria in DM7 for DAMIC status • • P. Privitera in DM7 and D. Baxter in DM4 for DAMIC-M update G. Gerbier in DM7 for NEWS-G updates • * This list is likely not complete. Apologies to those I didn’t call out. 6

  7. Clean assembly and operations are critical The picture can't be displayed. 7

  8. We are researching and developing shielding and low background construction The researchers that includes world leading expertise in low background materials. Real-time assay of radioactive fallout during construction. 8

  9. We are researching and developing radon abatement and assay 9

  10. An injection of 65M$ in Canada to support astroparticle physics Strengthen international collaborations. “ To be a globally recognized centre for research and learning, coalescing Canadian and international expertise in underground particle astrophysics and benefitting from the unique SNOLAB facility to deliver world-leading science focused on the big questions in particle astrophysics, cosmology and astronomy.” Numerous programs have been launched: - 15 new faculty members - About 85 research staff. Postdocs, students - Support for research – experiments and R&D - International programs include: - Support for visiting scientists/sabbaticals to or from Canada - A PhD exchange program. To give students the opportunity to gain experience at another institution in or outside Canada. (So far exchanges with Japan, Portugal, UK….) 10 https://mcdonaldinstitute.ca/

  11. Fin End

  12. LEGEND 1000 concept From talk by W. Pettus Next generation neutrino and dark matter experiments nEXO concept from talk by M. Heffner • Watching the Canadian community planning` process • Tonne-scale neutrinoless double-beta decay (DOE Nuclear Physics CD0) • Generation-3 Dark Matter (DOE High Energy Physics P5) • Dark Matter New Initiatives (DOE High Energy Physics Program) 12 From ‘Building for Discovery’ P5 report (2014)

  13. Laboratory Space • Strawman plan for laboratory expansion now exists • Cost for expansion is ~120M CAD • Not actively proposing to expand • Expect space allocations may be more competitive in the future 13

  14. SNOLAB includes a campus 2 km underground 14

  15. Why Science at SNOLAB is Underground Radiation is everywhere! Crab Pulsar, Hubble M87, Hubble Space and Chandra Space Telescope, NASA The Earth, Apollo 17, NASA Telescopes, NASA 15

  16. Back Background nds from super perno nova a re remnants and superm rmassive bla lack holes ho es in n und nder erground nd labo aborat atories es enabling low background science… S. Swordy 16

  17. SNOLAB people enable science SNOLAB has a focus on User Project Support • Scientific • Engineering • Construction • Operations Sudbury hosts a strong mining/industrial base that projects can draw from • Excavation • Fabrication • Integration Laurentian University is the Sudbury research 17 anchor for the user base

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