Signs of a non-zero equation-of-state for Dark Matter
Krishna Naidoo

TL;DR
This paper proposes a model with a negative, evolving dark matter equation-of-state that can resolve cosmological tensions and explains the ISW void anomaly, predicting observable effects on cosmic expansion and structure growth.
Contribution
It introduces a dark matter model with a negative EoS at late times, unifying dark sector effects and addressing current cosmological tensions.
Findings
Negative EoS increases Hubble constant
Reduces σ8, alleviating tensions
Predicts larger ISW effect at low redshift
Abstract
We demonstrate how a changing and negative equation-of-state (EoS) for dark matter can alleviate cosmic tensions and explain the integrated Sachs-Wolfe (ISW) void anomaly. We discuss the effect of the model on the cosmic expansion history, growth of structure and the ISW. We show that a negative EoS at late times is able to produce a larger Hubble constant and smaller , which can explain both cosmological tensions. Furthermore, the model uniquely predicts larger ISW at low redshift, a prediction which is in agreement with observations of larger ISW from voids. The preference for a negative EoS for dark matter at late times is indicative of a unified dark sector and degenerate with models of dark matter and dark energy interaction. Future measurements of the ISW from cosmic voids can provide a unique test for this solution to tensions in cosmology, should they continue to…
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Taxonomy
TopicsCosmology and Gravitation Theories · Advanced Thermodynamics and Statistical Mechanics · Astronomy and Astrophysical Research
