Constraining the dark matter-vacuum energy interaction using the EDGES 21-cm absorption signal
arXiv:1805.11210 · doi:10.3847/1538-4357/aaeb9c
Abstract
The recent measurement of the global 21-cm absorption signal reported by the Experiment to Detect the Global Epoch of Reionization Signature (EDGES) Collaboration is in tension with the prediction of the CDM model at a significance level. In this work, we report that this tension can be released by introducing an interaction between dark matter and vacuum energy. We perform a model parameter estimation using a combined dataset including EDGES and other recent cosmological observations, and find that the EDGES measurement can marginally improve the constraint on parameters that quantify the interacting vacuum, and that the combined dataset favours the CDM at 68\% CL. This proof-of-the-concept study demonstrates the potential power of future 21-cm experiments to constrain the interacting dark energy models.
6 pages, 5 figures, 1 table; accepted for publication in ApJ
References in corpus (20)
- The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
- Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe
- An absorption profile centred at 78 megahertz in the sky-averaged spectrum
- Baryon Acoustic Oscillations in the Lyα forest of BOSS DR11 quasars
- Possible interaction between baryons and dark-matter particles revealed by the first stars
- Insights on Dark Matter from Hydrogen during Cosmic Dawn
- Enhanced global signal of neutral hydrogen due to excess radiation at cosmic dawn
- Severely Constraining Dark Matter Interpretations of the 21-cm Anomaly
- The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: a tomographic measurement of cosmic structure growth and expansion rate based on optimal redshift weights
- Modeling the Radio Background from the First Black Holes at Cosmic Dawn: Implications for the 21 cm Absorption Amplitude
- Constraining Baryon--Dark Matter Scattering with the Cosmic Dawn 21-cm Signal
- The EDGES 21 cm Anomaly and Properties of Dark Matter
- How well do we understand cosmological recombination?
- Cosmological constraints on a decomposed Chaplygin gas
- Inhomogeneous vacuum energy
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space
- Post- constraints on interacting vacuum energy
- Interacting Dark Energy: Possible Explanation for 21-cm Absorption at Cosmic Dawn
- Can Early Dark Energy Explain EDGES?
- Can Conformal and Disformal Couplings Between Dark Sectors Explain the EDGES 21cm Anomaly?
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- Non-minimal dark sector physics and cosmological tensions
- Interacting dark energy in the early 2020s: a promising solution to the and cosmic shear tensions
- The Giant Radio Array for Neutrino Detection (GRAND): Science and Design
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- Listening to the sound of dark sector interactions with gravitational wave standard sirens
- Dark sectors with dynamical coupling
- Dawn of the dark: unified dark sectors and the EDGES Cosmic Dawn 21-cm signal
- Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
- Inflation and Early Dark Energy with a Stage II Hydrogen Intensity Mapping Experiment
- Implications of the possible 21-cm line excess at cosmic dawn on dynamics of interacting dark energy
- Tightening the reins on non-minimal dark sector physics: Interacting Dark Energy with dynamical and non-dynamical equation of state
- On the dynamics of a dark sector coupling
- Probing the effects of primordial black holes on 21-cm EDGES signal along with interacting dark energy and dark matter - baryon scattering
- Can Conformal and Disformal Couplings Between Dark Sectors Explain the EDGES 21cm Anomaly?
- Probing Interacting Dark Energy and Scattering of Baryons with Dark Matter in Light of EDGES 21cm Signal
- Observational constraints on the interacting dark energy - dark matter (IDM) cosmological models
- Interacting dark energy after DESI DR2: a challenge for CDM paradigm?
- Observational constraints on interacting vacuum energy with linear interactions
- On the interacting dark energy scenarios the case for Hubble constant tension
- Constraining structure formation using EDGES
- Global 21-cm brightness temperature in viscous dark energy models
- Interacting Dark Energy: New parametrization and observational constraints
- Implications of the cosmological 21-cm absorption profile for high-redshift star formation and deep JWST surveys
- Joint analysis of EDGES -cm line observations with standard candles and rulers in CDM and non-adiabatic gCg models