arXiv · 1905.01611
Hidden symmetries of two-field cosmological models
Abstract
We determine the most general time-independent Noether symmetries of two-field cosmological models with rotationally-invariant scalar manifold metrics. In particular, we show that such models can have hidden symmetries, which arise if and only if the scalar manifold metric has Gaussian curvature $-3/8$, i.e. when the model is of elementary $\alpha$-attractor type with a fixed value of the parameter $\alpha$. In this case, we find explicitly all scalar potentials compatible with hidden Noether symmetries, thus classifying all models of this type. We also discuss some implications of the corresponding conserved quantity.
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Lilia Anguelova, Elena Mirela Babalic, Calin Iuliu Lazaroiu. 2019-05-05. Hidden symmetries of two-field cosmological models. https://doi.org/10.1007/jhep09(2019)007
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