Evading the theoretical no-go theorem for nonsingular bounces in Horndeski/Galileon cosmology
Shreya Banerjee, Yi-Fu Cai, Emmanuel N. Saridakis

TL;DR
This paper demonstrates that nonsingular cosmological bounces free of ghosts and instabilities are possible within Horndeski and Galileon theories by relaxing previous assumptions, with explicit examples provided.
Contribution
It challenges the existing no-go theorem by showing that its assumptions can be violated, enabling nonsingular bounces in these theories.
Findings
Violating the assumption of continuity of a key quantity allows nonsingular bounces.
Considering cyclic cosmology can evade the theorem's restrictions.
Explicit models of nonsingular bounces without pathologies are constructed.
Abstract
We show that a nonsingular bounce, free of ghosts and gradient instabilities, can be realized in the framework of Horndeski or generalized Galileon cosmology. In particular, we first review that the theoretical no-go theorem, which states that the above is impossible, is based on two very strong assumptions, namely that a particular quantity cannot be discontinuous during the bounce, and that there is only one bounce. However, as we show in the present work, the first assumption not only can be violated in a general Horndeski/Galileon scenario, but also it is necessarily violated at the bounce point within the subclass of Horndeski/Galileon gravity in which becomes zero at . Additionally, concerning the second assumption, which is crucial in improved versions of the theorem which claim that even if a nonlinear free of pathologies can be realized it will lead to…
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