Simulations of cosmological scalar fields
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Updated
Jun 18, 2026 - Julia
Simulations of cosmological scalar fields
We provide a consistent description of the reheating era of a constrained Gauss-Bonnet model by using the same free parameters that result in a viable inflationary era. The theory predicts a propagation velocity of tensor perturbations which is equal to unity in order to be in agreement with the GW170817 event. The reheating era turns out to be …
Microscopic-closure audit showing imported gauge-radiation realizations recollapse or freeze and do not close a predictive S-brane child map.
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