IWDM: The fate of an interacting non-cold dark matter $-$ vacuum scenario
Supriya Pan, Weiqiang Yang, Eleonora Di Valentino, David F. Mota,, Joseph Silk

TL;DR
This study explores a cosmological model where dark matter has a variable, non-zero equation of state interacting with vacuum energy, using observational data to assess its viability and find a slight preference for non-cold dark matter.
Contribution
It introduces and tests an interacting non-cold dark matter-vacuum scenario with a variable dark matter equation of state using multiple observational datasets.
Findings
Non-zero dark matter equation of state is mildly preferred.
Data suggests possible deviation from cold dark matter assumption.
Further investigation into non-cold dark matter is warranted.
Abstract
In most cosmological models, the equation of state of the dark matter is assumed to be zero, which means that the dark matter is pressure-less or cold. While this hypothesis is based on the abundance of cold dark matter in the universe, however, there is no compelling reason to assume that the equation of state of dark matter is exactly zero. A more general approach would be to allow for a range of values for the dark matter equation of state and use the observational data to determine which values are most likely. With the increasing accuracy of experimental data, we have chosen to explore the possibility of interacting non-cold dark matter vacuum scenario, where the equation of state of the dark matter is constant but can take different values within a specific range. Using the Cosmic Microwave Background (CMB) anisotropies and the CMB lensing reconstruction from the Planck legacy…
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