New IceCube results next Thursday (June 29)

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SUMMARY

The IceCube Neutrino Observatory will present groundbreaking results on June 29, revealing high-energy neutrino emissions from the Milky Way. This research, conducted by the IceCube Collaboration, involved analyzing a dataset of 60,000 neutrinos collected over a decade, significantly improving sensitivity compared to previous studies. The findings confirm the Milky Way as a source of high-energy neutrinos, linking cosmic rays with galactic gas and dust interactions. The results will be published in the journal Science, providing new insights into cosmic phenomena.

PREREQUISITES
  • Understanding of high-energy astrophysics
  • Familiarity with neutrino detection technology
  • Knowledge of cosmic ray interactions
  • Basic comprehension of scientific research methodologies
NEXT STEPS
  • Research the IceCube Neutrino Observatory's detection methods
  • Study the implications of high-energy neutrinos in astrophysics
  • Explore the relationship between gamma rays and neutrinos in cosmic events
  • Read the published article in Science for detailed methodologies and findings
USEFUL FOR

Astronomers, astrophysicists, and researchers interested in high-energy particle physics and cosmic ray studies will benefit from this discussion.

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TL;DR
IceCube is a neutrino detector in Antarctica, looking for neutrino at the highest energies.
Join us to hear exciting IceCube results!

It'll involve neutrinos, but beyond that I don't know what it is about. It will be something important or they wouldn't make a press conference.

I don't expect a relation, but it's interesting that NANOGrav has some news the same day.
 
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Physics news on Phys.org
"the IceCube Neutrino Observatory has produced an image of the Milky Way using neutrinos—tiny, ghostlike astronomical messengers. In an article to be published tomorrow, June 30, in the journal Science, the IceCube Collaboration, an international group of over 350 scientists, presents evidence of high-energy neutrino emission from the Milky Way.

The high-energy neutrinos, with energies millions to billions of times higher than those produced by the fusion reactions that power stars, were detected by the IceCube Neutrino Observatory, a gigaton detector operating at the Amundsen-Scott South Pole Station. . . . unlike the case for light of any wavelength, in neutrinos, the universe outshines the nearby sources in our own galaxy. . . .

Interactions between cosmic rays—high-energy protons and heavier nuclei, also produced in our galaxy–and galactic gas and dust inevitably produce both gamma rays and neutrinos. Given the observation of gamma rays from the galactic plane, the Milky Way was expected to be a source of high-energy neutrinos. “A neutrino counterpart has now been measured, thus confirming what we know about our galaxy and cosmic ray sources. . . “The improved methods allowed us to retain over an order of magnitude more neutrino events with better angular reconstruction, resulting in an analysis that is three times more sensitive than the previous search,” . . . .

The dataset used in the study included 60,000 neutrinos spanning 10 years of IceCube data, 30 times as many events as the selection used in a previous analysis of the galactic plane using cascade events. These neutrinos were compared to previously published prediction maps of locations in the sky where the galaxy was expected to shine in neutrinos."

https://icecube.wisc.edu/news/press...ugh-a-new-lens-neutrinos-detected-by-icecube/
 
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