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001     295198
005     20211110133445.0
024 7 _ |a arXiv:1110.5837
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024 7 _ |a 10.3204/DESY-PROC-2011-04/cadamuro_davide
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024 7 _ |a inspire:943177
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037 _ _ |a PUBDB-2016-01114
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088 1 _ |a MPP-2011-124; arXiv:1110.5837
088 _ _ |a MPP-2011-124
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088 _ _ |a arXiv:1110.5837
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100 1 _ |a Cadamuro, Davide
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111 2 _ |a 7th Patras Workshop on Axions, WIMPs and WISPs
|g AXION-WIMP 2011
|c Mykonos
|d 2011-06-27 - 2011-07-01
|w Greece
245 _ _ |a Cosmological Constraints on Thermal Relic Axions and Axion-like Particles
260 _ _ |c 2011
300 _ _ |a 139-142
336 7 _ |a Conference Paper
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336 7 _ |a INPROCEEDINGS
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520 _ _ |a Cosmological precision data can be used to set very strict constraints on Axions and Axion-like particles (ALPs) produced thermally in the big bang. We briefly review the known bounds and propose two new constraints for Axions and ALPs decaying in the early universe, based upon the concomitant dilution of baryon and neutrino densities, using WMAP7 and other cosmological data.
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588 _ _ |a Dataset connected to INSPIRE
650 _ 7 |a axion: thermal
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650 _ 7 |a big bang
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650 _ 7 |a neutrino: density
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650 _ 7 |a WMAP
|2 INSPIRE
693 _ _ |a HERA
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700 1 _ |a Redondo, Javier
|b 1
773 _ _ |a 10.3204/DESY-PROC-2011-04/cadamuro_davide
787 0 _ |a Schumann, Marc et.al.
|d 2011
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|r DESY-PROC-2011-04
|t Proceedings, 7th Patras Workshop on Axions, WIMPs and WISPs
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