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Assuming both that our Universe is evolving into a de Sitter space and a vanishing cosmological constant, leaves only the option that the observed acceleration is provided by a "kinetic" energy of a scalar field.
doi:10.1007/BF01807638
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doi:10.1103/PhysRevLett.59.2607
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J. Martin, Everything You Always Wanted To Know About The Cosmological Constant Problem (But Were Afraid To Ask), Comptes Rendus Physique 13 (2012) 566–665 · 2012
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S. Appleby, E. V. Linder, The Paths of Gravity in Galileon Cosmology, JCAP 1203 (2012) 043 · 2012
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A. De Felice, S. Tsujikawa, Conditions for the cosmological viability of the most general scalar-tensor theories and their applications to extended Galileon dark energy models, JCAP 1202 (2012) 007 · 2012
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C. Charmousis, E. J. Copeland, A. Padilla, P. M. Saffin, Self-tuning and the derivation of a class of scalar-tensor theories, Phys. Rev. D85 (2012) 104040 · 2012
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C. Germani, L. Martucci, P. Moyassari, Introducing the Slotheon: a slow Galileon scalar field in curved space-time, Phys. Rev. D85 (2012) 103501 · 2012
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P. Martin-Moruno, N. J. Nunes, F. S. N. Lobo, Horndeski theories self-tuning to a de Sitter vacuum, Phys. Rev. D91 (8) (2015) 084029 · 2015
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P. Martin-Moruno, N. J. Nunes, Attracted to de Sitter II: cosmology of the shift-symmetric Horndeski models, JCAP 1509 (09) (2015) 056 · 2015
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C. Germani, Initial conditions for the Galileon dark energy, Phys. Dark Univ. 15 (2017) 1–6 · 2016
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