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Models of exponential and power-law acceleration of the Universe in Horndeski theory without ghosts and Laplace instabilities
We present a designer method for flat Friedman-Robertson-Walker space-times within the framework of Horndeski's scalar-tensor theory. As a result, one can find subclasses of Horndeski's scalar-tensor theory within which cosmological solutions exist without ghosts and Laplace instabilities. As an exa
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