| Home > Publications database > Cosmological Higgs-Axion Interplay for a Naturally Small Electroweak Scale` > print |
| 001 | 291990 | ||
| 005 | 20211110132704.0 | ||
| 024 | 7 | _ | |2 arXiv |a arXiv:1506.09217 |
| 024 | 7 | _ | |2 altmetric |a altmetric:4229781 |
| 024 | 7 | _ | |2 inspire |a inspire:1380474 |
| 037 | _ | _ | |a PUBDB-2015-05724 |
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| 082 | _ | _ | |a 550 |
| 088 | 1 | _ | |a arXiv:1506.09217 |
| 088 | _ | _ | |a arXiv:1506.09217 |2 arXiv |
| 100 | 1 | _ | |0 P:(DE-HGF)0 |a Espinosa, J. R. |b 0 |
| 245 | _ | _ | |a Cosmological Higgs-Axion Interplay for a Naturally Small Electroweak Scale` |
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| 520 | _ | _ | |a Recently, a new mechanism to generate a naturally small electroweak scale has been proposed. It exploits the coupling of the Higgs to an axion-like field and a long era in the early universe where the axion unchains a dynamical screening of the Higgs mass. We present a new realization of this idea with the new feature that it leaves no signs of new physics up to a rather large scale, 10^9 GeV, except for two very light and weakly coupled axion-like states. One of the scalars can be a viable Dark Matter candidate. Such a cosmological Higgs-axion interplay could be tested with a number of experimental strategies. |
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| 700 | 1 | _ | |0 P:(DE-HGF)0 |a Panico, G. |b 1 |
| 700 | 1 | _ | |0 P:(DE-HGF)0 |a Pomarol, A. |b 2 |
| 700 | 1 | _ | |0 P:(DE-HGF)0 |a Pujolàs, O. |b 3 |
| 700 | 1 | _ | |0 P:(DE-H253)PIP1023797 |a Servant, Geraldine |b 4 |u desy |
| 700 | 1 | _ | |0 P:(DE-H253)PIP1023796 |a Grojean, Christophe |b 5 |e Corresponding author |u desy |
| 856 | 4 | _ | |u http://arxiv.org/abs/1506.09217 |
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| 914 | 1 | _ | |y 2015 |
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