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Free keywords:
High Energy Physics - Theory, hep-th,Astrophysics, Cosmology and Extragalactic Astrophysics, astro-ph.CO,General Relativity and Quantum Cosmology, gr-qc
Abstract:
Ekpyrotic instantons describe the emergence of classical contracting
universes out of the no-boundary quantum state. However, up to now these
instantons ended in a big crunch singularity. We remedy this by adding a
higher-derivative term, allowing a ghost condensate to form. This causes a
smooth, non-singular bounce from the contracting phase into an expanding,
kinetic-dominated phase. Remarkably, and although there is a non-trivial
evolution during the bounce, the wavefunction of the universe is "classical" in
a WKB sense just as much after the bounce as before. These new non-singular
instantons can thus form the basis for a fully non-singular and calculable
ekpyrotic history of the universe, from creation until now.
