| Home > Publications database > Bounds on Very Weakly Interacting Sub-eV Particles (WISPs) from Cosmology and Astrophysics > print |
| 001 | 297010 | ||
| 005 | 20211110133938.0 | ||
| 024 | 7 | _ | |a 10.3204/DESY-PROC-2008-02/redondo_javier |2 datacite_doi |
| 024 | 7 | _ | |a arXiv:0810.3200 |2 arXiv |
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| 088 | 1 | _ | |a arXiv:0810.3200; DESY-08-130 |
| 088 | _ | _ | |a arXiv:0810.3200 |2 arXiv |
| 088 | _ | _ | |a DESY-08-130 |2 DESY |
| 100 | 1 | _ | |a Redondo, Javier |0 P:(DE-H253)PIP1006281 |b 0 |e Corresponding author |u desy |
| 111 | 2 | _ | |a 4th Patras Workshop on Axions, WIMPs and WISPs |g AXION-WIMP 2008 |c Hamburg |d 2008-06-18 - 2008-06-21 |w Germany |
| 245 | _ | _ | |a Bounds on Very Weakly Interacting Sub-eV Particles (WISPs) from Cosmology and Astrophysics |
| 260 | _ | _ | |c 2009 |b Deutsches Elektronen-Synchrotron, DESY |a Hamburg |
| 300 | _ | _ | |a 23-26 |
| 336 | 7 | _ | |a Conference Paper |0 33 |2 EndNote |
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| 520 | _ | _ | |a Many weakly interacting sub-electronVolt particles (WISPs) are easily accommodated in extensions of the standard model. Generally the strongest bounds on their existence come from stellar evolution and cosmology, where to the best of our knowledge observations seem to agree with the standard budget of particles. In this talk I review the most demanding constraints for axions and axion-like-particles, hidden photons and mini-charged particles. |
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| 773 | _ | _ | |a 10.3204/DESY-PROC-2008-02/redondo_javier |
| 787 | 0 | _ | |a Lindner, Axel et.al. |d Verlag Deutsches Elektronen-Synchrotron, 2008 |i IsPartOf |0 PUBDB-2016-01759 |r DESY-PROC-2008-02 |t Proceedings, 4th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2008) |
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