Interacting dark energy in the early 2020s: A promising solution to the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e1519" altimg="si57.svg"> <mml:msub> <mml:mrow> <mml:mi>H</mml:mi> </mml:mrow> <mml:mrow> <mml:mn>0</mml:mn> </mml:mrow> </mml:msub> </mml:math> and cosmic shear tensions
Eleonora Di Valentino, Alessandro Melchiorri, Olga Mena, Sunny Vagnozzi
Topics & Concepts
PhysicsDark energyCosmic microwave backgroundPlanckBaryon acoustic oscillationsHubble's lawAstrophysicsDark matterLambda-CDM modelGalaxyCOSMIC cancer databaseAstronomyAge of the universeObservational cosmologyCosmologyStructure formationMetric expansion of spaceCosmic background radiationCosmological constantPhysical cosmologyScalar field dark matterDark fluidVacuum energyUniverseShear (geology)Cold dark matterBaryonRedshiftGalaxy clusterHot dark matterDark radiationWarm dark matterCosmology and Gravitation TheoriesDark Matter and Cosmic PhenomenaGalaxies: Formation, Evolution, Phenomena