Diffuse ultrahigh-energy gamma-ray emission from TeV halos
Journal Article
·
· Physical Review. D.
- Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP)
- Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
- Univ. of Chicago, IL (United States)
- Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
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. Here, these results support the conclusion that TeV halos dominate the ultrahigh-energy sky, and that these objects convert of their total spindown power into very high and ultrahigh-energy photons.
- Research Organization:
- Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
- Sponsoring Organization:
- USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF)
- Grant/Contract Number:
- AC02-07CH11359
- OSTI ID:
- 1984947
- Report Number(s):
- FERMILAB-PUB--23-272-T; arXiv:2306.00051; oai:inspirehep.net:2664573
- Journal Information:
- Physical Review. D., Journal Name: Physical Review. D. Journal Issue: 8 Vol. 109; ISSN 2470-0010
- Publisher:
- American Physical Society (APS)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
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