Cosmological effect of coherent oscillation of ultralight scalar fields in a multicomponent universe
Priyanka Saha, Dipanjan Dey, Kaushik Bhattacharya

TL;DR
This paper develops a comprehensive method to model ultralight scalar fields as cold dark matter in complex, multicomponent cosmological settings, extending previous flat universe results to curved and interacting scenarios.
Contribution
It introduces a new general approach to represent ultralight scalar fields as CDM in multicomponent, curved universes, including non-minimal couplings and gravitational collapse.
Findings
Exact equivalence in flat FLRW without cosmological constant
Generalized equivalence in curved universes with multiple components
First-time modeling of scalar field collapse in closed FLRW universe
Abstract
The idea that coherent oscillations of a scalar field, oscillating over a time period that is much shorter than the cosmological timescale, can exhibit cold dark matter (CDM) like behavior was previously established. In our work we first show that this equivalence between the oscillating scalar field model and the CDM sector is exact only in a flat Friedmann-Lemaitre-Robertson-Walker (FLRW) spacetime in the absence of cosmological constant and any other possible matter components in the universe when the mass of the scalar field is very large compared to the Hubble parameter. Then we show how to generalize the equivalence between the coherently oscillating scalar field model and the CDM sector in a spatially curved universe with multiple matter components. Using our general method, we will show how a coherently oscillating scalar field model can represent the CDM sector in the presence…
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