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The KeV Majoron as a dark matter particle

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The KeV Majoron as a dark matter particle

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dc.contributor.author Berezinsky, Veniamin
dc.contributor.author Furtado Valle, José Wagner
dc.date.accessioned 2015-09-24T12:10:16Z
dc.date.available 2015-09-24T12:10:16Z
dc.date.issued 1993
dc.identifier.citation Berezinsky, Veniamin Furtado Valle, José Wagner 1993 The KeV Majoron as a dark matter particle Physics Letters B 318 2 360 366
dc.identifier.uri http://hdl.handle.net/10550/47223
dc.description.abstract We consider a very weakly interacting KeV majoron as dark matter particle (DMP), which provides both the critical density ρcr=1.88×10−29h2 g/cm3 and the galactic scale Mgal ∼m3Pl/m2J∼1012M⊙(mJ/1KeV)−2 for galaxy formation. The majoron couples to leptons only through some new 'directly interacting particles', called DIPS, and this provides the required smallness of the coupling constants. If the masses of these DIPS are greater than the scale Vs characterizing the spontaneous violation of the global lepton symmetry they are absent at the corresponding phase transition (T∼Vs) and the majorons are produced during the phase transition, never being in thermal equilibrium during the history of the universe. In the alternative case mDIP<Vs the majorons can be for a short period in thermal equilibrium. This scenario is not forbidden by nucleosynthesis and gives a reasonable growth factor for the density fluctuations compatible with COBE. A possible signature is an X-ray line at Eγ=mJ2, produced by the decay J→γ+γ. A model is described which realizes the possibility of the KeV majoron as DMP and may also lead to observable rates for decays such as $\mu \ra e \gamma$ and $\mu \ra 3e$.
dc.language.iso eng
dc.relation.ispartof Physics Letters B, 1993, vol. 318, num. 2, p. 360-366
dc.subject Física
dc.title The KeV Majoron as a dark matter particle
dc.type journal article es_ES
dc.date.updated 2015-09-24T12:10:17Z
dc.identifier.doi 10.1016/0370-2693(93)90140-D
dc.identifier.idgrec 073574
dc.rights.accessRights open access es_ES

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