Properties of singularities in the (phantom) dark energy universe
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- Type
- article
- Published
- 2005-01-05
- Cited by
- 1,046
- References
- 0
- Access
- Open access
- OpenAlex
- https://openalex.org/W1963581370
- Semantic Scholar
- https://api.semanticscholar.org/CorpusID:119103085
Keywords
Dark energy, Big Rip, Physics, Gravitational singularity, Phantom energy
References
Cited by
- Scalar perturbation of the viscosity dark fluid cosmological model
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- Brane Kantowski-Sachs universe with linear equation of state and a future singularity
- Holographic dark energy reconstruction in f(T,T)f(T,T) gravity
- Generalized second law of thermodynamics in f(T) gravity with entropy corrections
- Transition from quintessence to the phantom phase in the quintom model
- Casimir Effect Near the Future Singularity in Kaluza Klein Viscous Cosmology
- Interacting realization of cosmological singularities with variable vacuum energy
- Interacting Holographic Dark Energy, Future Singularity and Polytropic Gas Model of Dark Energy in Closed FRW Universe
- Dark energy from quantum gravity
- Cosmological dynamics and dark energy with a nonlinear equation of state: a quadratic model
- The osgood criterion and finite‐time cosmological singularities
- Study of non-canonical scalar field model using various parametrizations of dark energy equation of state
- Isotropic turbulence in the dark fluid universe with inhomogeneous equation of state
- Observational constraints on EoS parameters of emergent universe
- Quantisation of the holographic Ricci dark energy model
- On Singularities in Cosmic Inflation
- Friedmann Cosmology with a Generalized Equation of State and Bulk Viscosity
- Smooth dynamical crossing of the phantom divide line of a scalar field in simple cosmological models
- DILATON COUPLED QUINTESSENCE MODEL IN THE ω - ω′ PLANE
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