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Cosmic Bose dark matter

Iván Rodríguez-MontoyaDepartamento de Física, Centro de Investigación y de Estudios Avanzados del Instituto Politécnico Nacional, Apartado Postal 14-740, 07000 México, Distrito Federal, MexicoAbdel Pérez-LorenzanaDepartamento de Física, Centro de Investigación y de Estudios Avanzados del Instituto Politécnico Nacional, Apartado Postal 14-740, 07000 México, Distrito Federal, MexicoE. De La Cruz–BureloDepartamento de Física, Centro de Investigación y de Estudios Avanzados del Instituto Politécnico Nacional, Apartado Postal 14-740, 07000 México, Distrito Federal, MexicoY. Giraud–HéraudLaboratoire AstroParticule et Cosmologie (APC), CNRS: UMR 7164, Université Denis Diderot Paris 7, 10, rue Alice Domon et Leonie Duquet, 75205 Paris, FranceTonatiuh MatosDepartamento de Física, Centro de Investigación y de Estudios Avanzados del Instituto Politécnico Nacional, Apartado Postal 14-740, 07000 México, Distrito Federal, Mexico
2013en
ABI

Annotatsiya

It is known that cold and hot dark matter imprint opposed effects on the cosmological observables; naturally, it is often thought that they should be made of different kinds of particles. We point out, however, that a Bose-Einstein condensate could be the source of both components. In this framework, the mass and temperature constraints on hot dark matter contain fundamental information of cold dark matter. We discuss two scenarios: a gas made of bosons and a gas made of boson-antiboson pairs. We obtain constraints on the bosonic dark matter parameters from cosmological data and test the idea by probing the condition on the critical temperature of condensation, including a forecast for the Planck mission. We find that the bosonic dark matter picture is consistent with data in the boson scenario, while the boson-antiboson scenario might be increasingly interesting for future data surveys.

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