- Gamma-ray and neutrino diffuse emissions of the Galaxy above the TeV
- Journal of Physics: Conference Series
- Volume | Issue number
- 718 | 5
- Article number
- Number of pages
- Document type
- Faculty of Science (FNWI)
- Institute for Theoretical Physics Amsterdam (ITFA)
Conventional cosmic ray propagation models face problems reproducing the diffuse 7-ray spectrum measured by Fermi-LAT over the entire sky. Those models also fail to smoothly connect Fermi-LAT results with data above the TeV as those taken by Milagro in the inner Galactic plane. In this contribution we show that a representative model adopting a spatial dependent rigidity scaling of the diffusion coefficient can reproduce all those experimental results without spoiling the consistency with local cosmic-ray measurements. We use the same model to compute the diffuse neutrino emission of the Galaxy and compare it with IceCube and ANTARES results.
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- Other links
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- XIV International Conference on Topics in Astroparticle and Underground Physics (TAUP 2015): 7–11 September 2015, Torino, Italy
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