Fermi-LAT 17-Year Data Confirms Global 20-30 GeV Cosmic-Ray Spectral Break at 4.44 Sigma
The Fermi-LAT study delivers the first statistically decisive evidence that a 20-30 GeV spectral break is a global property of the Galactic disk. This finding directly ties gamma-ray emission to cosmic-ray propagation physics and reframes models of interstellar turbulence.
{"The analysis accounts for correlated instrumental systematics in diffuse gamma-ray emission along the Galactic plane. By modeling pion-decay dominance up to 100 GeV, the team isolates a slope change of Delta gamma approximately 0.20 that aligns precisely with local cosmic-ray spectra rather than regional variations.","This result overturns assumptions that cosmic-ray spectral hardening is a purely local phenomenon. Instead it supports a shift from Kolmogorov to Kraichnan turbulence as the driver, with implications for particle acceleration models at supernova remnants and the origin of the cosmic-ray knee at higher energies.","Prior Fermi analyses lacked the exposure and systematic control to establish the break globally. Cross-checks with AMS-02 and CREAM proton and helium data strengthen the multimessenger link, showing the feature is not an artifact of solar modulation or local sources.","Future tests require TeV-range mapping with CTA and IceCube neutrino correlations to confirm whether the same turbulence transition persists above the knee, falsifiable within three years if the break amplitude remains consistent."}
CTA Collaboration: Global spectral break amplitude will remain within 10 percent of Delta gamma = 0.20 in 1-10 TeV band by 2028 if turbulence transition model holds.
Sources (3)
- [1]Primary Source(https://arxiv.org/abs/2608.28757)
- [2]Supporting Source(https://arxiv.org/abs/2205.00343)
- [3]Supporting Source(https://doi.org/10.1103/PhysRevLett.125.251101)