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2016

Non-linear Fields in Generalized Cosmologies

Fasiello, Matteo, Vlah, Zvonimir

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The perturbative approach to structure formation has recently received a lot of attention in the literature.

In such setups the final predictions for observables like the power spectrum is often derived under additional approximations such as a simplified time dependence.
Here we provide all-order perturbative integral solutions for density and velocity fields in generalized cosmologies, with a direct application to clustering quintessence.
We go beyond the standard results based on extending the EdS-like approximations.

Non-linear Fields in Generalized Cosmologies · Around

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