Cosmological evolution of interacting dark energy in Lorentz violation
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Publication:982007
DOI10.1140/epjc/s10052-009-1104-1zbMath1189.83119arXiv0809.3847OpenAlexW3104635156MaRDI QIDQ982007
Freddy P. Zen, Arianto, Triyanta, Agus Purwanto, Bobby Eka Gunara
Publication date: 2 July 2010
Published in: The European Physical Journal C. Particles and Fields (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/0809.3847
Related Items (7)
Dynamical systems applied to cosmology: dark energy and modified gravity ⋮ Considering late-time acceleration in some cosmological models ⋮ Cosmological model with nonminimal derivative coupling of scalar fields in five dimensions ⋮ Modified gravitational equations on braneworld with Lorentz invariant violation ⋮ Kerr-Newman-NUT-Kiselev black holes in Rastall theory of gravity and Kerr/CFT correspondence ⋮ Interaction between tachyon and hessence (or hantom) dark energies ⋮ COSMOLOGICAL ASPECTS OF A VECTOR FIELD MODEL
Cites Work
- Perturbations and quasi-normal modes of black holes in Einstein-aether theory
- Unification of dark matter and dark energy: the inhomogeneous Chaplygin gas
- Cosmological constant -- the weight of the vacuum
- The fundamental constants and their variation: observational and theoretical status
- The cosmological constant and dark energy
- Vector field as a quintessence partner
- DYNAMICS OF DARK ENERGY
- Black holes in Einstein-aether theory
- Spherical solutions in Einstein-aether theory: static aether and stars
- FIELD THEORY OF TACHYON MATTER
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Cosmological Imprint of an Energy Component with General Equation of State
- The Cosmological Constants
- An alternative to quintessence
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