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IceCube Upgrade and Gen-2 Summer Blot for the IceCube-Gen2 - PowerPoint PPT Presentation

IceCube Upgrade and Gen-2 Summer Blot for the IceCube-Gen2 collaboration 26 August 2018 TeVPA - Berlin IceCube Neutrino Observatory A pioneering multi-purpose detector Astrophysics Discovery of astrophysical neutrinos First


  1. IceCube Upgrade and Gen-2 Summer Blot for the IceCube-Gen2 collaboration 26 August 2018 TeVPA - Berlin

  2. IceCube Neutrino Observatory A pioneering multi-purpose detector Astrophysics • Discovery of astrophysical neutrinos • First evidence for neutrino point source with TXS • Key partner in multi-messenger landscape • Cosmic rays with IceTop 
 Particle Physics • Atmospheric neutrino oscillations • Neutrino cross-sections at TeV-scale • Exotic/BSM physics searches 
 Spacing [m] Earth science Energy threshold [GeV] Horizontal Vertical • Glaciology • Earth tomography 125 17 ~100 IceCube 50 7 ~5 DeepCore | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 2

  3. IceCube limitations More potential to exploit! Angular resolution • Median error not scaling with photon statistics 
 Ice modelling systematic uncertainties • Bubble column distorts angular acceptance • Anisotropy of photon scattering and/or absorption lengths in ice Bore hole Still frame from Sweden camera Bubble 
 column | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 3

  4. The IceCube Upgrade The next step in precision astroparticle physics with IceCube IC Upgrade • 7 strings with ~20 m spacing • 2 m vertical spacing of 125 modules / string • Located inside of IceCube-DeepCore | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 4

  5. WOM The IceCube Upgrade - R&D small PMT In-situ testing of new optical modules adiabatic mDOM D-Egg PDOM light guide wavelength shifter coated cylinder Φ pressure housing 30 cm 36 cm 11 cm New sensor designs will incorporate one or more of the following: • Upgraded electronics • Smaller diameter • Increased UV acceptance • Larger and/or pixelated effective area | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 5

  6. The IceCube Upgrade - Calibration POCAM [3] Deployment of new devices at better distances Integrated devices Piezo-module [1] • LED flashers • Acoustic sensors • Optical cameras Stand-alone light sources • Precision Optical Calibration Module CCD [2] CMOS [2] (POCAM) • ns-pulsed LEDs with small opening angle Reduce primary systematic uncertainties • Better calibration of new and existing sensors • Improved knowledge of glacial ice [1] https://doi.org/10.1051/epjconf/201713506003 [2] https://doi.org/10.22323/1.301.1040 [3] https://doi.org/10.22323/1.301.0934 | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 6

  7. The IceCube Upgrade - Science Not just for calibration and R&D! High statistics sample over several orders of magnitude in energy FOR FREE! “Conventional flux” K + π + π 0 µ+ ν µ e + ν e Honda, et. al: https://arxiv.org/abs/1502.03916 | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 7

  8. The IceCube Upgrade - Science Precision atmospheric oscillation measurements Similar physics program to DeepCore, just better! • Oscillations, non-standard interactions, sterile neutrinos, dark matter… 500km (2018) Δ m 232 = 2.51 x 10 -3 eV 2 θ 23 = π /2 12,700km First order effect for 
 atmospheric neutrinos: | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 8

  9. The IceCube Upgrade - Science Precision atmospheric oscillation measurements Similar physics program to DeepCore, just better! • Oscillations, non-standard interactions, sterile neutrinos, dark matter… OPERA (68%) arxiv:1804.04912 Projected sensitivities do not include reduced ice/OM systematics | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 9

  10. IceCube-Gen 2 A vision for the future of neutrino astroparticle physics at the South Pole High energy Low energy • Precision measurements of • Find (more) neutrino point sources atmospheric neutrino oscillations: 
 • Characterise spectrum, flux, and ν µ →ν τ 
 flavour composition of astrophysical Neutrino mass ordering neutrinos with higher precision • Characterise atmospheric flux • GZK neutrinos (hadronic interactions) • Continue search for BSM physics • Also continue search for BSM physics | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 10

  11. IceCube-Gen 2 High energy facility In-Ice High Energy Array (HEA) • 120 strings with ~240 m spacing and 80 OMs each • 6.2 - 9.5 km 3 instrumented volume (not yet fixed) Surface array • Under investigation: Air Cherenkov Telescope (IceAct) vs scintillator panels • Prototypes of both systems deployed and operating at the South Pole Radio array Surface array High Energy Array PoS (ICRC2017) 991 | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 11

  12. High Energy Array Projected sensitivity • Improved angular resolution • Better point sensitivity, here shown for 15 y IC86 + 15 y IC-Gen2 • Discovery potential ~2.5x better than sensitivity • Surface veto (assumed 75 km 2 ) improves sensitivity (discovery potential) by factor ~3 PoS (ICRC2017) 991 | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 12

  13. IceCube-Gen 2 100 m Low energy facility Precision IceCube Next Generation Upgrade (PINGU) • 26 strings with ~20-30 m spacing and 125 OMs each • Profit from surrounding 86-strings of IceCube-DeepCore as cosmic muon veto • Lower energy threshold to ~100 MeV IC86 PINGU | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 13

  14. Neutrino oscillations Highest energy probe of atmospheric ν µ →ν τ mixing Expected precision: Δ m 232 ~ 1% (1 σ ) θ 23 ~ 4% (1 σ ) depends on NMO and true θ 23 | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 14

  15. Neutrino oscillations Neutrino Mass Ordering PINGU LOI Version 2 @ arXiv:1401.2046v2 | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 15

  16. The IceCube-Gen 2 Facility Preliminary timeline 2016 2017 2018 2019 2020 2021 2022 2023 2024 2025 2026 … 2032 Deployment IceCube Upgrade Construction R&D Design & Approval Surface air shower Today Radio array IC86 Surface array IceCube Upgrade PINGU High Energy Array MeV- to EeV-scale physics | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 16

  17. The future is bright for the next generation of IceCube Thank you for your attention!

  18. Backup

  19. Timeline in project years 19

  20. Atmospheric neutrino physics Neutrino oscillations Flavour states Mass states (not equal) Atmospheric Reactor Solar Accelerator Accelerator Reactor First order effect for 
 atmospheric neutrinos: | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 20

  21. Neutrino oscillations Vacuum oscillations *Normal mass ordering assumed θ 23 = π /2 Δ m 232 = 2.51 x 10 -3 eV 2 | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 21

  22. Neutrino oscillations Including matter effects *Normal mass ordering assumed θ 23 = π /2 Δ m 232 = 2.51 x 10 -3 eV 2 | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 22

  23. A probe for new physics The matter matters! New Physics • Unitarity of PMNS matrix • Non-standard interactions • Flavour changing • Cross-section enhancement • Environmental decoherence PRL 118, 221801 (2017) | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 23

  24. The global picture Putting things in context IceCube Collaboration, J.Phys. G44 (2017) no.5 | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 24

  25. Neutrino oscillations See talk by T. DeYoung Neutrino Astronomy 5 DeepCore NuMu Disappearance | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 25

  26. Neutrino oscillations See talk by T. DeYoung Neutrino Astronomy 5 DeepCore NuTau Appearance | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 26

  27. Ice anisotropy South Pole ice anisotropy: Proceedings of ICRC2013 0580, 2014 Data Simulation | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 27

  28. The IceCube Upgrade - Calibration Example: POCAM triangulation and characterisation of bubble column https://doi.org/10.22323/1.301.0934 | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 28

  29. The IceCube Upgrade - Science Improved reconstruction of high energy interactions Improved cascade angular resolution Improved identification of astrophysical ν τ • Use POCAMs to mimic double-bang with 20m spacing • Reduced uncertainty on ice anisotropy Tianlu Yuan, TeVPA 2018 | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 29

  30. https://arxiv.org/pdf/1412.5106.pdf 30

  31. Improved physics reach with new sensors 31

  32. High Energy Array Precise measurement of diffuse flux PoS (ICRC2017) 991 | IceCube Upgrade and Gen2 | Summer Blot | TeVPA 2018 32

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