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• W3208363532 endingPage "100899" @default.
• W3208363532 startingPage "100899" @default.
• W3208363532 abstract "In this work we consider a scenario where the dark energy is a dynamical fluid whose energy density can be transferred to the dark matter via a coupling function proportional to the energy density of the dark energy. In particular, we investigate this model’s ability to address the S8 tension and find that against data from Planck, BAO and Pantheon the model (1) can significantly reduce the significance of the tension, (2) does so without exacerbating nor introducing any other tension (such as the H0 tension) and (3) without worsening the fit to the considered data sets with respect to the ΛCDM model. We also test the model against data from weak lensing surveys such as KiDS and DES, and find that the model’s ability to address the S8 tension further improves, without a significant impact on any other parameter nor statistical measure." @default.
• W3208363532 created "2021-11-08" @default.
• W3208363532 creator A5007550660 @default.
• W3208363532 date "2021-12-01" @default.
• W3208363532 modified "2023-10-17" @default.
• W3208363532 title "Dark energy–dark matter interactions as a solution to the <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline id=d1e1043 altimg=si5.svg><mml:msub><mml:mrow><mml:mi>S</mml:mi></mml:mrow><mml:mrow><mml:mn>8</mml:mn></mml:mrow></mml:msub></mml:math> tension" @default.
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• W3208363532 doi "https://doi.org/10.1016/j.dark.2021.100899" @default.
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