Axion Dark Matter and Cosmological Parameters
arXiv:1104.4507 · doi:10.1103/PhysRevLett.108.061304
Abstract
We observe that photon cooling after big bang nucleosynthesis (BBN) but before recombination can remove the conflict between the observed and theoretically predicted value of the primordial abundance of Li. Such cooling is ordinarily difficult to achieve. However, the recent realization that dark matter axions form a Bose-Einstein condensate (BEC) provides a possible mechanism, because the much colder axions may reach thermal contact with the photons. This proposal predicts a high effective number of neutrinos as measured by the cosmic microwave anisotropy spectrum.
4 pages, one figure. Version to appear in Phys. Rev. Lett., incorporating useful comments by the referees and emphasizing that photon cooling by axion BEC is a possibility, not a certainty
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- Cosmological solutions to the Lithium problem: Big-bang nucleosynthesis with photon cooling, -particle decay and a primordial magnetic field
- Cosmological Inhomogeneities with Bose-Einstein Condensate Dark Matter
- Natural explanation for 21cm absorption signals via axion-induced cooling
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- Constraints on Bose-Einstein-condensed Axion Dark Matter from The HI Nearby Galaxy Survey data
- Cosmology of an Axion-Like Majoron
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- A Solution to Lithium Problem by Long-Lived Stau
- A detailed exploration of the EDGES 21 cm absorption anomaly and axion-induced cooling
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