Searching for dark matter - dark energy interactions: going beyond the conformal case
Carsten van de Bruck, Jurgen Mifsud

TL;DR
This paper investigates non-gravitational interactions between dark matter and dark energy, constraining their possible couplings using current cosmological data, and finds no strong evidence for such interactions.
Contribution
It provides the first comprehensive constraints on conformal, disformal, and mixed dark sector interactions using multiple cosmological observations.
Findings
No significant evidence for dark sector interactions.
Growth of structure data improves parameter constraints.
Local Hubble constant value does not affect interaction constraints.
Abstract
We consider a generic cosmological model which allows for non-gravitational direct couplings between dark matter and dark energy. The distinguishing cosmological features of these couplings can be probed by current cosmological observations, thus enabling us to place constraints on this generic interaction which is composed of the conformal and disformal coupling functions. We perform a global analysis in order to independently constrain the conformal, disformal, and mixed interactions between dark matter and dark energy by combining current data from: Planck observations of the cosmic microwave background radiation anisotropies, a combination of measurements of baryon acoustic oscillations, a supernovae Type Ia sample, a compilation of Hubble parameter measurements estimated from the cosmic chronometers approach, direct measurements of the expansion rate of the Universe today, and a…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
