2011
DOI: 10.1088/1475-7516/2011/01/004
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Cosmic antiproton constraints on effective interactions of the dark matter

Abstract: Using an effective interaction approach to describe the interactions between the dark matter particle and the light degrees of freedom of the standard model, we calculate the antiproton flux due to the annihilation of the dark matter in the Galactic Halo and compare to the most recent antiproton spectrum of the PAMELA experiment. We obtain useful constraints on the size of the effective interactions that are comparable to those deduced from collider and gamma-ray experiments.

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Cited by 35 publications
(39 citation statements)
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“…For instance, refs. [32][33][34][35][36][37][38] study operators relevant to specific indirect DM searches, while ref. [39] offers a global fit including also direct searches, collider constraints and cosmological limits.…”
Section: Jhep12(2015)120mentioning
confidence: 99%
“…For instance, refs. [32][33][34][35][36][37][38] study operators relevant to specific indirect DM searches, while ref. [39] offers a global fit including also direct searches, collider constraints and cosmological limits.…”
Section: Jhep12(2015)120mentioning
confidence: 99%
“…Similarly, constraints from indirect searches can be interpreted in these models on the plane of direct detection [31][32][33]. We enlarge our previous set of effective theories to allow couplings to only one type of quarks at a time.…”
Section: Introductionmentioning
confidence: 99%
“…Effective operators are also useful as a way to compare the strength of indirect detection constraints with constraints from other searches such as direct detection experiments and colliders [25,31,48,[163][164][165].…”
Section: Effective Field Theories For Indirect Detectionmentioning
confidence: 99%