# Cosmology from multimeasure multifield model

## TL;DR

This paper explores a unified cosmological model that combines inflation, dark energy, dark matter, and the Higgs mechanism, demonstrating through numerical analysis that it can describe the entire Universe evolution with some model adjustments.

## Contribution

It reformulates a recently proposed model using effective measures into a quintessential framework and shows its capability to model the full cosmic history with improved dynamics.

## Key findings

- The model can describe the entire Universe evolution seamlessly.
- Effective friction in the model leads to finite-time inflation with low slow-roll parameters.
- Predicts a constant scalar field in the late Universe.

## Abstract

We consider the cosmological application of a (variant of) relatively newly proposed model \cite{1609.06915} unifying inflation, dark energy, dark matter, and the Higgs mechanism. The model was originally defined using additional non-Riemannian measures but it can be reformulated into effective quintessential model unifying inflation, dark energy and dark matter. Here we demonstrate numerically that it is capable of describing the entire Universe evolution in a seamless way, but this requires some revision of the model setup. The main reason is that there is a strong effective friction in the model, a feature which has been neglected in the pioneer work. This improves the model potential for proper description of the Universe evolution, because the friction ensures a finite time inflation with dynamically maintained low-value slow-roll parameters in the realistic scenarios. In addition, the model predicts the existence of a constant scalar field in late Universe.