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Recently the PAMELA experiment has released its updated anti-proton flux and anti-proton to proton flux ratio data up to energies of ~200GeV.
- With no clear excess of cosmic ray anti-protons at high energies, one can extend constraints on the production of anti-protons from dark matter.
- In this letter, we consider both the cases of dark matter annihilating and decaying into standard model particles that produce significant numbers of anti-protons.
- We provide two sets of constraints on the annihilation cross-sections/decay lifetimes.
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