Show simple item record

dc.contributor.authorBai, Yang
dc.contributor.authorSu, Meng
dc.contributor.authorZhao, Yue
dc.date.accessioned2014-04-24T20:18:17Z
dc.date.available2014-04-24T20:18:17Z
dc.date.issued2013-02
dc.identifier.issn1029-8479
dc.identifier.issn1126-6708
dc.identifier.urihttp://hdl.handle.net/1721.1/86238
dc.description.abstractBoth the robust INTEGRAL 511 keV gamma-ray line and the recent tentative hint of the 135 GeV gamma-ray line from Fermi-LAT have similar signal morphologies, and may be produced from the same dark matter annihilation. Motivated by this observation, we construct a dark matter model to explain both signals and to accommodate the two required annihilation cross sections that are different by more than six orders of magnitude. In our model, to generate the low-energy positrons for INTEGRAL, dark matter particles annihilate into a complex scalar that couples to photon via a charge-radius operator. The complex scalar contains an excited state decaying into the ground state plus an off-shell photon to generate a pair of positron and electron. Two charged particles with non-degenerate masses are necessary for generating this charge-radius operator. One charged particle is predicted to be long-lived and have a mass around 3.8 TeV to explain the dark matter thermal relic abundance from its late decay. The other charged particle is predicted to have a mass below 1 TeV given the ratio of the two signal cross sections. The 14 TeV LHC will concretely test the main parameter space of this lighter charged particle.en_US
dc.description.sponsorshipUniversity of Wisconsin--Madison (Start-up funds)en_US
dc.description.sponsorshipSLAC National Accelerator Laboratory (US DOE contract DE-AC02-76SF00515)en_US
dc.description.sponsorshipAspen Center for Physics (NSF Grant No. 1066293)en_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration (Einstein Postdoctoral Fellowship grant number PF2-130102)en_US
dc.description.sponsorshipSmithsonian Astrophysical Observatory (Chandra X-ray Center, NASA under contract NAS8-03060)en_US
dc.language.isoen_US
dc.publisherSpringer-Verlag/International School for Advanced Studies (SISSA)en_US
dc.relation.isversionofhttp://dx.doi.org/10.1007/jhep02(2013)097en_US
dc.rightsCreative Commons Attributionen_US
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/en_US
dc.sourceSpringeren_US
dc.titleDichromatic dark matteren_US
dc.typeArticleen_US
dc.identifier.citationBai, Yang, Meng Su, and Yue Zhao. “Dichromatic Dark Matter.” J. High Energ. Phys. 2013, no. 2 (February 2013).en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.mitauthorSu, Mengen_US
dc.relation.journalJournal of High Energy Physicsen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsBai, Yang; Su, Meng; Zhao, Yueen_US
mit.licensePUBLISHER_CCen_US
mit.metadata.statusComplete


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record