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We study the gravitational wave (GW) production in extremely strong first order phase transitions where the latent heat density dominates the plasma energy density, $\alpha \gtrsim 1$.
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1985
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1999
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2001
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A. Kosowsky, A. Mack, and T. Kahniashvili, “Gravitational radiation from cosmological turbulence,”
2002
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A. Nicolis, “Relic gravitational waves from colliding bubbles and cosmic turbulence,”
2004
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G. M. Harry, P. Fritschel, D. A. Shaddock, W. Folkner, and E. S. Phinney, “Laser interferometry for the big bang observer,”
2006
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2006
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2007
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2008
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R. Jinno and M. Takimoto, “Probing a classically conformal B-L model with gravitational waves,”
2017
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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,”
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2008
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2009
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D. Bodeker and G. D. Moore, “Can electroweak bubble walls run away?,”
2009
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2010
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2010
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2011
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D. E. Morrissey and M. J. Ramsey-Musolf, “Electroweak baryogenesis,”
2012
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2017
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R. Jinno and M. Takimoto, “Gravitational waves from bubble collisions: An analytic derivation,”
2017
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2017
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2018
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B. von Harling and G. Servant, “QCD-induced Electroweak Phase Transition,”
2018
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2018
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2018
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T. Konstandin, “Gravitational radiation from a bulk flow model,”
2018
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2018
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2019
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2019
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T. Prokopec, J. Rezacek, and B. wieewska, “Gravitational waves from conformal symmetry breaking,”
2019
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2019
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P. Baratella, A. Pomarol, and F. Rompineve, “The Supercooled Universe,”
2019
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R. Jinno and M. Takimoto, “Gravitational waves from bubble dynamics: Beyond the Envelope,”
2019
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A. Kosowsky, M. S. Turner, and R. Watkins, “Gravitational waves from first order cosmological phase transitions,”
2029
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