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COT3 - Nonsingular Cosmology

Speaker

Olmo Alba, Gonzalo

Co-autors

Carlos Barragán, Hèlios Sanchis-Alepuz

Talk Title

Avoiding the Big Bang singularity with Palatini f(R) theories.

Abstract

We discuss the conditions that guarantee the existence of homogeneous and isotropic models that avoid the Big Bang singularity in $f(R)$ theories in Palatini formalism. We show that for such models the Big Bang singularity can be replaced by a cosmic bounce without violating any energy condition. In fact, the bounce is possible even for presureless dust. We give a characterization of such models and discuss their dynamics in the region near the bounce. We also find that power-law lagrangians with a finite number of terms may lead to non-singular universes, which contrasts with the infinite-series Palatini $f(R)$ lagrangian that one needs to fully capture the effective dynamics of Loop Quantum Cosmology.

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