2016
DOI: 10.5817/ah2016-2-23
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Příspěvek k mobilitě v kamnářském řemesle

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Cited by 4 publications
(3 citation statements)
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“…Phenomenologically, axion masses in the range we have constrained [approximately H 0 < m a < H(z eq )], and up to 10 −23 eV, are probed by the CMB power spectrum and large scale structure [27,59,60]. Higher masses in the range 10 −22 eV m a 10 −20 eV are motivated by their interesting effects on galaxy formation [13,44,[61][62][63], and are probed by high redshift galaxy formation [64][65][66][67] and the Lyman-alpha forest flux power spectrum [68,69].…”
Section: Discussionmentioning
confidence: 96%
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“…Phenomenologically, axion masses in the range we have constrained [approximately H 0 < m a < H(z eq )], and up to 10 −23 eV, are probed by the CMB power spectrum and large scale structure [27,59,60]. Higher masses in the range 10 −22 eV m a 10 −20 eV are motivated by their interesting effects on galaxy formation [13,44,[61][62][63], and are probed by high redshift galaxy formation [64][65][66][67] and the Lyman-alpha forest flux power spectrum [68,69].…”
Section: Discussionmentioning
confidence: 96%
“…While inflation is well-motivated by cosmological observations, it is unlikely to be possible to determine the theory precisely due to the limited information available. Dark matter, on the other hand, offers far greater prospects for precision measurement [60], and so by studying multiaxion models in the late Universe we might discover more about physics beyond the Standard Model. In this work we have presented the first exploration of a random matrix multi-axion model for dark matter and dark energy and have used statistical methods to bound the axion mass and decay constant distributions.…”
Section: Discussionmentioning
confidence: 99%
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