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We extend the matter bounce scenario to a more general theory in which the background dynamics and cosmological perturbations are generated by a $k$-essence scalar field with an arbitrary sound speed.
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2010
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T. Qiu, J. Evslin, Y. F. Cai, M. Li and X. Zhang, “Bouncing Galileon Cosmologies,” JCAP 1110
2011
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D. A. Easson, I. Sawicki and A. Vikman, “G-Bounce,” JCAP 1111
2011
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C. Burrage, C. de Rham, D. Seery and A. J. Tolley, “Galileon inflation,” JCAP 1101
2011
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2015
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Y. F. Cai and E. Wilson-Ewing, “A Λ \Lambda CDM bounce scenario,” JCAP 1503
2015
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