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A rather minimal possibility is that dark matter consists of the gauge bosons of a spontaneously broken symmetry.
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2009
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M. Punturo et al., The Einstein Telescope: A third-generation gravitational wave observatory , Class. Quant. Grav. 27
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2016
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2016
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F. Kahlhoefer, Review of LHC Dark Matter Searches , Int. J. Mod. Phys. A 32
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2010
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2010
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2010
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2011
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T. Regimbau, The astrophysical gravitational wave stochastic background , Res. Astron. Astrophys. 11
2011
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P. A. Rosado, Gravitational wave background from binary systems , Phys. Rev. D 84
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2011
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2012
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2017
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2017
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2017
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D. Bodeker and G. D. Moore, Electroweak Bubble Wall Speed Limit , JCAP 1705
2017
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2017
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2017
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2017
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2017
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2017
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2017
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M. Aoki, H. Goto and J. Kubo, Gravitational Waves from Hidden QCD Phase Transition , Phys. Rev. D 96
2017
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2017
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2018
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T. Hambye, A. Strumia and D. Teresi, Super-cool Dark Matter , JHEP 08
2018
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2018
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2018
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2018
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2018
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2018
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B. von Harling and G. Servant, QCD-induced Electroweak Phase Transition , JHEP 01
2018
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2018
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2018
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2019
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A. Kosowsky, M. S. Turner and R. Watkins, Gravitational waves from first order cosmological phase transitions , Phys. Rev. Lett. 69
2029
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