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- W1500564103 abstract "We explore the viability of a boson dark matter candidate with an asymmetry between the number densities of particles and antiparticles. A simple thermal field theory analysis confirms that, under certain general conditions, this component would develop a Bose-Einstein condensate in the early universe that, for appropriate model parameters, could survive the ensuing cosmological evolution until now. The condensation of a dark matter component in equilibrium with the thermal plasma is a relativistic process, hence the amount of matter dictated by the charge asymmetry is complemented by a hot relic density frozen out at the time of decoupling. Contrary to the case of ordinary WIMPs, dark matter particles in a condensate must be lighter than a few tens of eV so that the density from thermal relics is not too large. Big-Bang nucleosynthesis constrains the temperature of decoupling to the scale of the QCD phase transition or above. This requires large dark matter-to-photon ratios and very weak interactions with standard model particles." @default.
- W1500564103 created "2016-06-24" @default.
- W1500564103 creator A5056360022 @default.
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- W1500564103 date "2016-04-11" @default.
- W1500564103 modified "2023-10-01" @default.
- W1500564103 title "Asymmetric condensed dark matter" @default.
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- W1500564103 doi "https://doi.org/10.1088/1475-7516/2016/04/019" @default.
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