Scalar field dark matter and dark energy: a hybrid model for the dark sector
DOI10.1088/1475-7516/2023/07/019zbMath1528.83060arXiv2211.13653MaRDI QIDQ6116507
Carsten Van De Bruck, Elsa M. Teixeira, Unnamed Author
Publication date: 18 July 2023
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2211.13653
modified gravitydark matter theorydark energy theorycosmological perturbation theory in GR and beyond
Unified quantum theories (81V22) Relativistic cosmology (83F05) Quantum optics (81V80) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Perturbations in context of PDEs (35B20) Dark matter and dark energy (83C56)
Cites Work
- Unnamed Item
- Unnamed Item
- Dynamical systems applied to cosmology: dark energy and modified gravity
- Radiation of scalar modes and the classical double copy
- A transition between bouncing hyper-inflation to ΛCDM from diffusive scalar fields
- Probing the imprints of generalized interacting dark energy on the growth of perturbations
- Dark Energy, Dark Matter and baryogenesis from a model of a complex axion field
- Unified Dark Matter, Dark Energy and baryogenesis via a “cosmological wetting transition”
- Coupled quintessence with a ΛCDM background: removing the σ8 tension
- Observational constraints and predictions of the interacting dark sector with field-fluid mapping
This page was built for publication: Scalar field dark matter and dark energy: a hybrid model for the dark sector