Cosmology with a Continuous Tower of Scalar Fields
Jose Beltr\'an Jim\'enez, David F. Mota, Paulo Santos

TL;DR
This paper explores a universe model with a continuous spectrum of scalar fields that can explain both dark matter and dark energy phenomena, showing how different mass modes dominate at various cosmic epochs.
Contribution
It introduces a novel cosmological model with a continuous tower of scalar fields, demonstrating their dual role in dark matter and dark energy evolution.
Findings
Heavy modes dominate early universe, mimicking matter.
Light modes dominate late universe, causing acceleration.
The model can unify dark matter and dark energy behaviors.
Abstract
We study the cosmological evolution for a universe in the presence of a continuous tower of massive scalar fields which can drive the current phase of accelerated expansion of the universe and, in addition, can contribute as a dark matter component. The tower consists of a continuous set of massive scalar fields with a gaussian mass distribution. We show that, in a certain region of the parameter space, the {\it heavy} modes of the tower (those with masses much larger than the Hubble expansion rate) dominate at early times and make the tower behave like the usual single scalar field whose coherent oscillations around the minimum of the potential give a matter-like contribution. On the other hand, at late times, the {\it light} modes (those with masses much smaller than the Hubble expansion rate) overcome the energy density of the tower and they behave like a perfect fluid with equation…
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