28 May 2018 to 1 June 2018
Gran Sasso Science Institute
Europe/Rome timezone
The workshop schedule is now available.

Difference between cosmic ray spectra in molecular clouds and in diffuse gas can explain the FERMI GeV excess

30 May 2018, 14:30
40m
Main Lecture Hall (Gran Sasso Science Institute)

Main Lecture Hall

Gran Sasso Science Institute

Viale Francesco Crispi 7, 67100 L'Aquila (Italy)

Speaker

Wim De Boer (KIT)

Presentation materials

There are no materials yet.