Please use this identifier to cite or link to this item: https://dspace.iiti.ac.in/handle/123456789/8436
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dc.contributor.authorRakshit, Subhenduen_US
dc.date.accessioned2022-03-17T01:00:00Z-
dc.date.accessioned2022-03-21T11:16:52Z-
dc.date.available2022-03-17T01:00:00Z-
dc.date.available2022-03-21T11:16:52Z-
dc.date.issued2016-
dc.identifier.citationMajumdar, D., Modak, K. P., & Rakshit, S. (2016). A two-component dark matter model with real singlet scalars confronting GeV γ-ray excess from galactic centre and fermi bubble. Pramana - Journal of Physics, 86(2), 343-351. doi:10.1007/s12043-015-1154-xen_US
dc.identifier.issn0304-4289-
dc.identifier.otherEID(2-s2.0-84959298670)-
dc.identifier.urihttps://doi.org/10.1007/s12043-015-1154-x-
dc.identifier.urihttps://dspace.iiti.ac.in/handle/123456789/8436-
dc.description.abstractWe propose a two-component dark matter (DM) model, each component of which is a real singlet scalar, to explain results from both direct and indirect detection experiments. We put the constraints on the model parameters from theoretical bounds, PLANCK relic density results and direct DM experiments. The γ-ray flux is computed from DM annihilation in this framework and is then compared with the Fermi-LAT observations from galactic centre region and Fermi bubble. © Indian Academy of Sciences.en_US
dc.language.isoenen_US
dc.publisherIndian Academy of Sciencesen_US
dc.sourcePramana - Journal of Physicsen_US
dc.subjectGalaxiesen_US
dc.subjectDark matteren_US
dc.subjectFermi bubbleen_US
dc.subjectFermi-LATen_US
dc.subjectGalactic centresen_US
dc.subjectGamma-ray fluxen_US
dc.subjectIndirect detectionen_US
dc.subjectModel parametersen_US
dc.subjectTheoretical boundsen_US
dc.subjectGamma raysen_US
dc.titleA two-component dark matter model with real singlet scalars confronting GeV γ-ray excess from galactic centre and Fermi bubbleen_US
dc.typeJournal Articleen_US
Appears in Collections:Department of Physics

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