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dc.contributor.authorDokuchaev, V
dc.contributor.authorBerezinsky, V
dc.contributor.authorEroshenko, Y
dc.contributor.authorKachelriess, Michael
dc.contributor.authorSolberg, Marius Aase
dc.date.accessioned2019-10-08T11:08:17Z
dc.date.available2019-10-08T11:08:17Z
dc.date.created2012-01-15T12:55:38Z
dc.date.issued2011
dc.identifier.citationPoS - Proceedings of Science. 2011, PoS(IDM2010) .nb_NO
dc.identifier.issn1824-8039
dc.identifier.urihttp://hdl.handle.net/11250/2620881
dc.description.abstractWe describe the cosmological scenario for the formation of superdense dark matter clumps. As an interesting particular example the case of superheavy neutralino as DMparticles is considered. The small-scale superdense clumps form from a non-standard spiky spectrum of perturbations during the radiation dominated era. These clumps are not destroyed by tidal interactions and can be extremely dense. Superdense clumps can be observed by the gamma-radiation from dark matter annihilations and by the gravitational wave detectors, while the overproduction of primordial black holes constrains this scenario.nb_NO
dc.language.isoengnb_NO
dc.publisherSissa Medialabnb_NO
dc.rightsNavngivelse-Ikkekommersiell-DelPåSammeVilkår 4.0 Internasjonal*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/deed.no*
dc.titleSuperdense dark matter clumpsnb_NO
dc.typeJournal articlenb_NO
dc.typePeer reviewednb_NO
dc.description.versionpublishedVersionnb_NO
dc.source.pagenumber4nb_NO
dc.source.volumePoS(IDM2010)nb_NO
dc.source.journalPoS - Proceedings of Sciencenb_NO
dc.identifier.cristin885974
dc.description.localcodeCopyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licencenb_NO
cristin.unitcode194,66,20,0
cristin.unitnameInstitutt for fysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1


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Navngivelse-Ikkekommersiell-DelPåSammeVilkår 4.0 Internasjonal
Except where otherwise noted, this item's license is described as Navngivelse-Ikkekommersiell-DelPåSammeVilkår 4.0 Internasjonal