2009
DOI: 10.1103/physrevlett.102.071301
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Constraints on WIMP Dark Matter from the High Energy PAMELAp¯/pData

Abstract: A new calculation of thep/p ratio in cosmic rays is compared to the recent PAMELA data. The good match up to 100 GeV allows to set constraints on exotic contributions from thermal WIMP dark matter candidates. We derive stringent limits on possible enhancements of the WIMP p flux: a mWIMP=100 GeV (1 TeV) signal cannot be increased by more than a factor 6 (40) without overrunning PAMELA data. Annihilation through the W + W − channel is also inspected and crosschecked with e + /(e − + e + ) data. This scenario is… Show more

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Cited by 246 publications
(221 citation statements)
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“…3 we also comment upon the consistency of these scenarios in the light of the new diffuse gamma ray data, as a specific application of the general constraints derived above. We limit ourselves to modes of annihilation in a pair of charged lepton final states at tree level since, on one hand, they appear the only ones not excluded by other constraints (most notably antiproton fraction [8,9]), on the other hand they are significantly less model-dependent than scenarios with annihilations proceeding via additional, non SM states [10]. For the case of decaying DM, which has been invoked as alternative explanation of the lepton anomalies, a fortiori we limit ourselves to leptonic channels.…”
Section: Introductionmentioning
confidence: 99%
“…3 we also comment upon the consistency of these scenarios in the light of the new diffuse gamma ray data, as a specific application of the general constraints derived above. We limit ourselves to modes of annihilation in a pair of charged lepton final states at tree level since, on one hand, they appear the only ones not excluded by other constraints (most notably antiproton fraction [8,9]), on the other hand they are significantly less model-dependent than scenarios with annihilations proceeding via additional, non SM states [10]. For the case of decaying DM, which has been invoked as alternative explanation of the lepton anomalies, a fortiori we limit ourselves to leptonic channels.…”
Section: Introductionmentioning
confidence: 99%
“…The measured p/ p ratio is claimed to be a factor of 2 -3× larger than predicted by secondary cosmic-ray production models constrained by, for example, the positron fraction e + /(e + +e − ) and the B/C ratio [5]. Given the associated rising positron fraction [2] at 10 GeV, which is often explained as due to additional sources like pulsars, and not from enhanced cosmic-ray induced production, one may ask whether there is a consistent explanation for the overabundantp and the enhanced positron fraction.…”
Section: Introductionmentioning
confidence: 99%
“…First is that ratiosp/ p and e + /(e + + e − ) are far less useful than the particle spectral intensities themselves [37], particularly when looking at fits to data using models involving multiple source populations. Second is that the model [5] showing a discrepancy with the AMS-02 data, used to constrain fits for dark matter candidates top production, was tailored to fit PAMELA data that becomes increasingly uncertain at high energies.…”
Section: 6p/ P Ratiomentioning
confidence: 99%
“…Since no excess of antiprotons over what is expected from conventional astrophysics is evident, these measurements can be used to place bounds on properties of dark matter; this has been done in several earlier works (see, for instance, [6,13,14,15,16]). As an illustration of our results, we recalculate these bounds using the propagation model of Section 4.…”
Section: Effect On Pamela Constraintsmentioning
confidence: 99%