4–6 May 2015
Union South
US/Central timezone

Session

Diffuse Neutrinos & Gamma Rays - Complementary Views on the High-Energy Universe

4 May 2015, 14:30
Union South

Union South

1308 West Dayton Street, Madison, WI 53706

Presentation materials

  1. Markus Ackermann (o=desy-zeuthen,ou=Institutions,dc=icecube,dc=wisc,dc=edu)
    04/05/2015, 14:30
    Diffuse Neutrinos & Gamma Rays - Complementary Views on the High-Energy Universe, Markus Ackermann, DESY
    Non-thermal processes in our cosmos have been studied for several decades through the observation of individual sources and diffuse emission in γ rays. However, the universe is transparent to γ rays only at MeV and GeV energies. Above 100 GeV, they are increasingly absorbed in interactions with the omnipresent radiation background from stars and the CMB. At TeV energies γ-ray observations are...
    Go to contribution page
Building timetable...