Updated
Updated · CGTN · Apr 29
DAMPE satellite finds charge-dependent cosmic ray acceleration limit
Updated
Updated · CGTN · Apr 29

DAMPE satellite finds charge-dependent cosmic ray acceleration limit

10 articles · Updated · CGTN · Apr 29
  • A Nature study using 2016-2024 data from China's Wukong satellite also points to a natural "super particle accelerator" about 1,000 light-years from Earth.
  • Researchers led by the Purple Mountain Observatory mapped protons, helium, carbon, oxygen and iron, finding all spectra drop sharply at high-energy thresholds set by particle charge, not mass.
  • The result provides the first direct evidence for a 1961 theory, builds on DAMPE's earlier 15-teravolt softening findings, and may help trace cosmic-ray origins and dark matter with 18.5 billion recorded events.
How does proving this 60-year-old cosmic ray theory refine our models of star formation and galactic magnetic fields?
A cosmic 'super accelerator' is suspected 1,000 light-years away. Can astronomers now pinpoint this source in our galactic neighborhood?
If cosmic ray acceleration is limited by charge, what does this reveal about the galaxy’s powerful ‘super accelerators’?

Confirming the Peters Cycle: DAMPE Reveals Charge-Scaling Cosmic Ray Acceleration Limits

Overview

In April 2026, the DAMPE satellite team published a landmark study revealing that cosmic-ray spectral softening occurs at energies scaling linearly with particle charge, confirming rigidity as the key factor in cosmic-ray acceleration and propagation. This discovery provided the first direct proof of the Peters cycle, showing that particles reach a charge-dependent maximum energy before escaping their source, likely a nearby accelerator such as a supernova remnant or pulsar. Enabled by DAMPE's advanced instrumentation and over a decade of data collection, these precise measurements bridge observational gaps and reduce uncertainties in ground-based experiments. DAMPE's findings reshape astrophysics, improving dark matter searches, particle physics models, and our understanding of galaxy evolution, while inspiring future cosmic-ray observatories.

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