Scaling solutions and weak gravity in dark energy with energy and momentum couplings
We argue that the ΛCDM tensions of the Hubble-Lemaȋtre expansion rate H0 and the clustering normalization σ8 can be eased, at least in principle, by considering an interaction between dark energy and dark matter in such a way to induce a small and positive early effective equation of state and a we...
Guardado en:
| Autores principales: | , |
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| Formato: | Article (Journal) |
| Lenguaje: | inglés |
| Publicado: |
9 June 2020
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| In: |
Journal of cosmology and astroparticle physics
Year: 2020, Número: 06 |
| ISSN: | 1475-7516 |
| DOI: | 10.1088/1475-7516/2020/06/020 |
| Acceso en línea: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1088/1475-7516/2020/06/020
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| Notas de Autor: | Luca Amendola and Shinji Tsujikawa |
| Sumario: | We argue that the ΛCDM tensions of the Hubble-Lemaȋtre expansion rate H0 and the clustering normalization σ8 can be eased, at least in principle, by considering an interaction between dark energy and dark matter in such a way to induce a small and positive early effective equation of state and a weaker gravity. For a dark energy scalar field ϕ interacting with dark matter through an exchange of both energy and momentum, we derive a general form of the Lagrangian allowing for the presence of scaling solutions. In a subclass of such interacting theories, we show the existence of a scaling ϕ-matter-dominated-era (ϕMDE) which can potentially alleviate the H0 tension by generating an effective high-redshift equation of state. We also study the evolution of perturbations for a model with ϕMDE followed by cosmic acceleration and find that the effective gravitational coupling relevant to the linear growth of large-scale structures can be smaller than the Newton gravitational constant G at low redshifts. The momentum exchange between dark energy and dark matter plays a crucial role for realizing weak gravity, while the energy transfer is also required for the existence of ϕMDE. |
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| Notas: | Gesehen am 01.09.2020 |
| Descripción Física: | Online Resource |
| ISSN: | 1475-7516 |
| DOI: | 10.1088/1475-7516/2020/06/020 |