Skip to Content

Search: {{$root.lsaSearchQuery.q}}, Page {{$root.page}}

Skip to Page Content
  2. ...
  3. DEPARTMENT COLLOQUIUM | IceCube and the Discovery of High-Energy Cosmic Neutrinos
    1. News and Events
    2. All Events
    3. Archived Events
    4. Department Colloquia
    5. 2015 Department Colloquia
  2. [X] close

DEPARTMENT COLLOQUIUM | IceCube and the Discovery of High-Energy Cosmic Neutrinos

  2. All News & Features
  3. All Events
    1. Archived Events
      1. 2013
      2. 2012
      3. 2011
      4. 2010
      5. 2009
      6. 2008
      7. 2007
      8. 2006
      9. 2005
      11. 2003
      12. 2002
      13. 2001
      14. 2000
      15. 1999
      16. HEP Astro
      17. Astronomy Colloquium
      18. Biophysics Seminar
      19. CM - AMO Seminars
      20. CM Theory Seminars
      21. Complex Systems
      22. Department Colloquia
        1. 2016 Department Colloquia
        2. 2015 Department Colloquia
        3. 2014 Department Colloquia
        4. 2013 Department Colloquia
        5. 2012 Department Colloquia
        6. 2011 Department Colloquia
        7. 2010 Department Colloquia
        8. 2009 Department Colloquia
        9. 2008 Department Colloquia
      24. Quantitative Biology Seminars
      25. HET Brown Bag Series
      26. HET Seminars
      27. Life After Grad School Seminars
      28. Farrand Memorial Lecture
      29. Workshops & Conferences
      30. Miscellaneous
      31. Saturday Morning Physics
      32. Special Lectures
      33. Search Events
  5. Special Lectures
  6. K-12 Programs
  7. Saturday Morning Physics
  8. Seminars & Colloquia
Wednesday, October 28, 2015
4:00 AM
340 West Hall

The IceCube project has transformed one cubic kilometer of natural Antarctic ice into a neutrino detector. The instrument detects more than 100,000 neutrinos per year in the GeV to PeV energy range. Among those, we have recently isolated a flux of high-energy cosmic neutrinos. I will discuss the instrument, the analysis of the data, and the significance of the discovery of cosmic neutrinos. The high cosmic neutrino flux observed indicates that a significant fraction of the radiation in the non-thermal universe, powered by compact objects from neutron stars to supermassive black holes, is generated by proton accelerators.

Speaker:
Physics
Randall Lab and Homer A. Neal Lab
450 Church Street
Ann Arbor, MI 48109-1040
734.764.4437
734.763.9694
Sitemap
© 2025 Regents of the University of Michigan