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Publikováno v:
Phys. Rev. D 108, 123524 (2023)
In Starobinsky inflation with a Weyl squared Lagrangian $-\alpha C^2$, where $\alpha$ is a coupling constant, we study the linear stability of cosmological perturbations on a spatially flat Friedmann-Lema\^{i}tre-Robertson-Walker background. In this
Externí odkaz:
http://arxiv.org/abs/2309.01835
