Accounting for the Unresolved X-ray Background with Sterile Neutrino Dark Matter

Simple item page
dc.creatorCumberbatch, Daniel
dc.creatorSilk, Joseph
dc.date2007-09-03
dc.date.accessioned2026-07-07T10:57:17Z
dc.date.available2026-07-07T10:57:17Z
dc.descriptionWe consider a scenario where keV sterile neutrinos constitute all of the currently inferred dark matter abundance, whose radiative decays could potentially account for the flux contributions to the X-ray background attributed to unresolved sources. Here we apply integrated flux methods to results from the observations of the North and South Chandra deep fields in order to deduce constraints on the sterile neutrino mass-mixing parameters.
dc.descriptionTo be published in the conference proceedings for the ''13th International Symposium on Particles, Strings and Cosmology'' (PASCOS-07), by the American Institute of Physics (AIP)
dc.identifierhttps://arxiv.org/abs/0709.0279
dc.identifierhttp://arxiv.org/abs/0709.0279
dc.identifierAIPConf.Proc.957:375-378,2007
dc.identifierdoi:10.1063/1.2823805
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/186705
dc.subjectAstrophysics
dc.titleAccounting for the Unresolved X-ray Background with Sterile Neutrino Dark Matter
dc.typetext

Files

Collections

arXiv