Weak cosmic growth in coupled dark energy with a lagrangian formulation

Ryotaro Kase, Shinji Tsujikawa

Research output: Contribution to journalArticlepeer-review

Abstract

We investigate a dark energy scenario in which a canonical scalar field φ is coupled to the four velocity uµc of cold dark matter (CDM) through a derivative interaction uµcµφ. The coupling is described by an interacting Lagrangian f(X, Z), where f depends on X = −∂µφ∂µφ/2 and Z = uµcµφ. We derive stability conditions of linear scalar perturbations for the wavelength deep inside the Hubble radius and show that the effective CDM sound speed is close to 0 as in the standard uncoupled case, while the scalar-field propagation speed is affected by the interacting term f. Under a quasi-static approximation, we also obtain a general expression of the effective gravitational coupling felt by the CDM perturbation. We study the late-time cosmological dynamics for the coupling f ∝ X(2−n)/2Zn and show that the gravitational coupling weaker than the Newton constant can be naturally realized for n > 0 on scales relevant to the growth of large-scale structures. This allows the possibility for alleviating the tension of σ8 between low- and high-redshift measurements.

Original languageEnglish
JournalUnknown Journal
Publication statusPublished - 2019 Nov 5

ASJC Scopus subject areas

  • General

Fingerprint Dive into the research topics of 'Weak cosmic growth in coupled dark energy with a lagrangian formulation'. Together they form a unique fingerprint.

Cite this