Theory of interacting vector dark energy and fluid
From MaRDI portal
Publication:6659009
DOI10.1088/1475-7516/2024/10/105MaRDI QIDQ6659009
Kazuya Koyama, Masroor C. Pookkillath
Publication date: 8 January 2025
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Cites Work
- Derivative self-interactions for a massive vector field
- Elastic perturbation theory in general relativity and a variation principle for a rotating solid star
- Variational aspects of relativistic field theories, with application to perfect fluids
- Addressing \(H_0\) tension by means of VCDM
- Massive gravity
- Vector field as a quintessence partner
- Action functionals for relativistic perfect fluids
- Hamiltonian formulation for multi-constituent relativistic perfect fluids
- Neutrino-assisted early dark energy: theory and cosmology
- Disformal map and Petrov classification in modified gravity
- Minimal theory of massive gravity and constraints on the graviton mass
- Coupled vector dark energy
- Reducing the H0 tension with generalized Proca theory
- Cosmology of Extended Proca-Nuevo
- The cosmological constant problem
- Relativistic fluid dynamics: physics for many different scales
- Observational bounds on extended minimal theories of massive gravity: new limits on the graviton mass
This page was built for publication: Theory of interacting vector dark energy and fluid
Report a bug (only for logged in users!)Click here to report a bug for this page (MaRDI item Q6659009)