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We argue that dark energy with multiple fields is theoretically well-motivated and predicts distinct observational signatures, in particular when cosmic acceleration takes place along a trajectory that is highly non-geodesic in field space.
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Gia Dvali, Stefan Hofmann, and Justin Khoury, “Degravitation of the cosmological constant and graviton width,” Phys. Rev. D 76
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Adam R. Brown, “Hyperbolic Inflation,” Phys. Rev. Lett. 121
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Sumit K. Garg and Chethan Krishnan, “Bounds on Slow Roll and the de Sitter Swampland,” JHEP 11
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