IceCube neutrino analysis pegs possible galactic source for cosmic rays

*********************************
There is now a CONTENT FREEZE for Mercury while we switch to a new platform. It began on Friday, March 10 at 6pm and will end on Wednesday, March 15 at noon. No new content can be created during this time, but all material in the system as of the beginning of the freeze will be migrated to the new platform, including users and groups. Functionally the new site is identical to the old one. webteam@gatech.edu
*********************************

External News Details

Scientists with the IceCube Neutrino Observatory in Antarctica have now analyzed a decade's worth of such neutrino detections and discovered evidence that an active galaxy called Messier 77 (aka the Squid Galaxy) is a strong candidate for one such high-energy neutrino emitter, according to a new paper published in the journal Science. It brings astrophysicists one step closer to resolving the mystery of the origin of high-energy cosmic rays. The IceCube international collaboration of scientists includes Ignacio Taboada, professor in the School of Physics who also serves as IceCube's spokesperson. (Coverage of this story also appears at Space.com, MSN.com, the Wall Street Journal (registration required), Phys.org, CNET, SciTechDaily, and Inverse.)

Additional Information

Groups

College of Sciences

Categories
Physics and Physical Sciences
Keywords
College of Sciences, School of Physics, Ignacio Taboada, IceCube Neutrino Observatory, neutrinos, gamma rays, Messier 77
Status
  • Created By: Renay San Miguel
  • Workflow Status: Published
  • Created On: Nov 7, 2022 - 3:25pm
  • Last Updated: Nov 18, 2022 - 4:58pm