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We study the decay of gravitational waves into dark energy fluctuations $\pi$, taking into account the large occupation numbers.
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P. Creminelli and F. Vernizzi, “Dark Energy after GW170817 and GRB170817A,”
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G. Gubitosi, F. Piazza, and F. Vernizzi, “The Effective Field Theory of Dark Energy,”
2013
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J. Gleyzes, D. Langlois, F. Piazza, and F. Vernizzi, “Essential Building Blocks of Dark Energy,”
2013
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E. Bellini and I. Sawicki, “Maximal freedom at minimum cost: linear large-scale structure in general modifications of gravity,”
2014
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J. Gleyzes, D. Langlois, F. Piazza, and F. Vernizzi, “Healthy theories beyond Horndeski,”
2015
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J. Gleyzes, D. Langlois, and F. Vernizzi, “A unifying description of dark energy,”
2015
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D. Pirtskhalava, L. Santoni, E. Trincherini, and F. Vernizzi, “Weakly Broken Galileon Symmetry,”
2015
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2017
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D. Langlois, M. Mancarella, K. Noui, and F. Vernizzi, “Effective Description of Higher-Order Scalar-Tensor Theories,”
2017
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P. Adshead, J. T. Giblin, and Z. J. Weiner, “Non-Abelian gauge preheating,”
2017
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P. Creminelli, M. Lewandowski, G. Tambalo, and F. Vernizzi, “Gravitational Wave Decay into Dark Energy,”
2018
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C. de Rham and S. Melville, “Gravitational Rainbows: LIGO and Dark Energy at its Cutoff,”
2018
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G. Cusin, M. Lewandowski, and F. Vernizzi, “Nonlinear Effective Theory of Dark Energy,”
2018
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L. Santoni, E. Trincherini, and L. G. Trombetta, “Behind Horndeski: Structurally Robust Higher Derivative EFTs,”
2018
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