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Galaxy.
Because the cosmic rays eventually escape the supernova remnant, they can only be accelerated up
to a certain maximum energy, which depends upon the size of the acceleration region and the
magnetic field strength.
However, cosmic rays have been observed at much higher energies than supernova remnants can
generate, and where these ultra-high-energies come from is a big question. Perhaps they come from
outside the Galaxy, from active galactic nuclei, quasars or gamma ray bursts. Or perhaps they're the
signature of some exotic new physics: superstrings, exotic dark matter, strongly-
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interactingneutrinos, or topological defects in the very structure of the universe. Questions like
these tie cosmic-ray astrophysics to basic particle physics and the fundamental nature of the
universe.
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