Velocity-dependent interacting dark energy and dark matter with a Lagrangian description of perfect fluids

Jose Beltran Jimenez, Dario Bettoni, David Figueruelo, Florencia A. Teppa Pannia, Shinji Tsujikawa

研究成果: Article査読

3 被引用数 (Scopus)

抄録

We consider a cosmological scenario where the dark sector is described by two perfect fluids that interact through a velocity-dependent coupling. This coupling gives rise to an interaction in the dark sector driven by the relative velocity of the components, thus making the background evolution oblivious to the interaction and only the perturbed Euler equations are affected at first order. We obtain the equations governing this system with the Schutz-Sorkin Lagrangian formulation for perfect fluids and derive the corresponding stability conditions to avoid ghosts and Laplacian instabilities. As a particular example, we study a model where dark energy behaves as a radiation fluid at high redshift while it effectively becomes a cosmological constant in the late Universe. Within this scenario, we show that the interaction of both dark components leads to a suppression of the dark matter clustering at late times. We also argue the possibility that this suppression of clustering together with the additional dark radiation at early times can simultaneously alleviate the σ8 and H0 tensions.

本文言語English
論文番号085
ジャーナルJournal of Cosmology and Astroparticle Physics
2021
3
DOI
出版ステータスPublished - 2021 3

ASJC Scopus subject areas

  • 天文学と天体物理学

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