Exploring a new interaction between dark matter and dark energy using the growth rate of structure
Mart\'in G. Richarte, Lixin Xu

TL;DR
This paper investigates a phenomenological interaction between dark matter and dark energy using a scale factor power law, analyzing its effects on cosmic structure growth and cosmic microwave background data to constrain the interaction parameters.
Contribution
It introduces a new scale factor power law interaction model between dark matter and dark energy and constrains its parameters using multiple cosmological datasets.
Findings
Large coupling constant favored by data.
Negative power law exponent preferred, affecting acoustic peaks.
Interaction shifts matter-radiation equality and alters power spectra.
Abstract
We present a phenomenological interaction with a scale factor power law form which leads to the appearance of two kinds of perturbed terms, a scale factor spatial variation along with perturbed Hubble expansion rate. We study both the background and the perturbation evolution within the parametrized post-Friedmann scheme, obtaining that the exchange of energy-momentum can flow from dark energy to dark matter in order to keep dark energy and dark matter densities well defined at all times. We combine several measures of the cosmic microwave background (WMAP9+Planck) data, baryon acoustic oscillation measurements, redshift-space distortion data, JLA sample of supernovae, and Hubble constant for constraining the coupling constant and the exponent provided both parametrized the interaction itself. The joint analysis of data seems to favor large…
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.
Taxonomy
TopicsCosmology and Gravitation Theories · Dark Matter and Cosmic Phenomena · Scientific Research and Discoveries
