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dc.date.accessioned2016-01-13T14:41:34Z
dc.date.available2016-01-13T14:41:34Z
dc.date.issued2014
dc.identifier.urihttp://hdl.handle.net/10852/48565
dc.description.abstractWe investigate the production of antideuterons from decaying dark matter, using gravitinos in supersymmetric models with trilinear R-parity-violating (RPV) operators as an example. The model used for antideuteron formation is shown to induce large uncertainties in the predicted flux, comparable to uncertainties from cosmic-ray propagation models. We improve on the formation model by tuning hadronization and coalescence parameters in Monte Carlo simulations to better reproduce the hadron spectra relevant for antideuteron production. In light of current bounds on fluxes and future prospects from the AMS-02 and GAPS experiments we set limits on RPV couplings as a function of the gravitino mass. © 2014 American Physical Societyen_US
dc.language.isoenen_US
dc.relation.ispartofDal, Lars Andreas (2015) Cosmic Ray Antideuterons from Particle Dark Matter. Doctoral thesis. http://urn.nb.no/URN:NBN:no-52442
dc.relation.urihttp://urn.nb.no/URN:NBN:no-52442
dc.titleAntideuteron limits on decaying dark matter with a tuned formation modelen_US
dc.typeJournal articleen_US
dc.creator.authorDal, Lars Andreas
dc.creator.authorRaklev, Are
dc.identifier.jtitlePhysical Review D
dc.identifier.volume89
dc.identifier.doihttp://dx.doi.org/10.1103/PhysRevD.89.103504
dc.identifier.urnURN:NBN:no-52437
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/48565/1/PhysRevD-89-103504.pdf
dc.type.versionPublishedVersion
cristin.articleid103504


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