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Interacting dark energy in the early 2020s: A promising solution to the H0 and cosmic shear tensions

  • Published:2020-12 Issue: Volume:30 Page:100666
  • ISSN:2212-6864
  • Container-title:Physics of the Dark Universe
  • language:en
  • Short-container-title:Physics of the Dark Universe

Author:

Di Valentino Eleonora,Melchiorri Alessandro,Mena Olga,Vagnozzi Sunny

Funder

European Research Council

TASP

PROMETEO

MINECO

European Union’s Horizon 2020 research and innovation programme

Isaac Newton Trust

Kavli Foundation

Homerton College, University of Cambridge

ESA Member States, NASA, and Canada

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference300 articles.

1. Observational evidence from supernovae for an accelerating universe and a cosmological constant;Riess;Astron. J.,1998

2. Measurements of Omega and Lambda from 42 high redshift supernovae;Perlmutter;Astrophys. J.,1999

3. Planck 2015 results. XIII. Cosmological parameters;Ade;Astron. Astrophys.,2015

4. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample;Alam;Mon. Not. R. Astron. Soc.,2017

5. Dark Energy Survey year 1 results: Cosmological constraints from cosmic shear;Troxel;Phys. Rev.,2018

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