AMS-02 and Next-to-Minimal Universal Extra Dimensions

Abstract

The anomaly detected by AMS-02 and PAMELA in the cosmic-ray positron flux when interpreted as arising from dark matter annihilation suggests that dark matter may interact differently with hadrons and leptons so as to remain compatible with cosmic-ray antiproton data. Such a scenario is readily accommodated in models with extra spatial dimensions. We study indirect detection of Kaluza-Klein (KK) dark matter in Universal Extra Dimensions with brane-localized terms and fermion bulk masses: Next-to-Minimal Universal Extra Dimensions. So that an excess of antiprotons is not produced in explaining the positron anomaly, it is necessary that the KK bulk masses in the lepton and hadron sectors be distinct. Even so, we find that cosmic-ray data disfavor a heavy KK photon dark matter scenario. Also, we find these scenarios with flavor-universal bulk masses to be in conflict with dijet and dilepton searches at the LHC.

5 pages, 3 figures

References in corpus (5)

• PYTHIA 6.4 Physics and Manual
• Observation of an anomalous positron abundance in the cosmic radiation
• The galactic antiproton spectrum at high energies: background expectation vs. exotic contributions
• Non-minimal universal extra dimensions
• Dark matter and pulsar signals for Fermi LAT, PAMELA, ATIC, HESS and WMAP data

Cited by in corpus (6)

• Electroweak Kaluza-Klein Dark Matter
• Leptophilic Dark Matter and AMS-02 Cosmic-ray Positron Flux
• A Review on Non-Minimal Universal Extra Dimensions
• Notes on sphere-based universal extra dimensions
• Fat brane, dark matter and localized kinetic terms in six dimensions
• Constraining Bosonic Supersymmetry from Higgs results and 8 TeV ATLAS multi-jets plus missing energy data