Stable or Unstable Light Dark Matter

Ma E.; Murthy M.V.N.; Rajasekaran G.

dc.contributor.author	Ma E.
dc.contributor.author	Murthy M.V.N.
dc.contributor.author	Rajasekaran G.
dc.date.accessioned	2023-11-03T11:57:30Z
dc.date.available	2023-11-03T11:57:30Z
dc.date.issued	2015
dc.identifier	10.48550/arXiv.1507.07609
dc.identifier.uri	https://dspace.imsc.res.in/xmlui/handle/123456789/828
dc.identifier.uri	https://doi.org/10.48550/arXiv.1507.07609
dc.description.abstract	We consider the case of light dark matter (∼10 GeV). We discuss a simple Z2 model of scalar self-interacting dark matter, as well as a related model of unstable long-lived dark matter which can explain the anomalous Kolar events observed decades ago.
dc.language.iso	en
dc.relation.ispartof	arXiv
dc.rights	Open Access
dc.source	arXiv
dc.subject	High Energy Physics - Phenomenology
dc.title	Stable or Unstable Light Dark Matter
dc.description.pages	1 - 7
dc.relation.url	https://doi.org/10.48550/arXiv.1507.07609
dc.publisher	arXiv
dc.type	article