arXiv · 2306.00051
Diffuse Ultra-High-Energy Gamma-Ray Emission From TeV Halos
Abstract
The LHAASO Collaboration has recently reported a measurement of the diffuse gamma-ray emission from the Galactic Plane at energies between 10 TeV and 1 PeV. While this emission is brighter than that expected from cosmic-ray interactions in the interstellar medium alone, we show that the intensity, spectrum, and morphology of this excess are in good agreement with that predicted from the "TeV halos" which surround the Milky Way's pulsar population. These results support the conclusion that TeV halos dominate the ultra-high-energy sky, and that these objects convert $\sim 5\%$ of their total spindown power into very-high and ultra-high-energy photons.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Ariane Dekker, Ian Holst, Dan Hooper, Giovani Leone, Emily Simon, Huangyu Xiao. 2023-05-31. Diffuse Ultra-High-Energy Gamma-Ray Emission From TeV Halos. https://doi.org/10.1103/physrevd.109.083026
Cite the original work for its findings. Save a collection to share your selection of sources.