Pages that link to "Item:Q2443610"
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The following pages link to Dark energy model with variable \(q\) and \(\omega\) in LRS Bianchi-II space-time (Q2443610):
Displaying 15 items.
- Anisotropic viscous fluid cosmological models from deceleration to acceleration in string cosmology (Q379264) (← links)
- Dark energy model in anisotropic Bianchi type-III space-time with variable eos parameter (Q416144) (← links)
- LRS Bianchi-I anisotropic cosmological model with dominance of dark energy (Q422255) (← links)
- Nonlinear spinor fields in Bianchi type-I spacetime reexamined (Q461834) (← links)
- Magnetised strings in \(\lambda\)-dominated anisotropic universe (Q517611) (← links)
- Dark energy models in plane symmetric space-time with time varying \(\varLambda \) term (Q1945619) (← links)
- \(\Lambda\) CDM-type cosmological model and observational constraints (Q2348662) (← links)
- Holographic dark energy model with quintessence in Bianchi type-I space-time (Q2391977) (← links)
- Holographic dark energy (DE) cosmological models with quintessence in Bianchi type-V space time (Q2436476) (← links)
- Early decelerating \& late time accelerating anisotropic cosmological models with dynamical EoS parameter (Q2442757) (← links)
- Accelerating universe with binary mixture of dark energy and perfect fluid in LRS Bianchi-V space-time (Q2516173) (← links)
- Scenario of two-fluid dark energy models in Bianchi type-III Universe (Q4615072) (← links)
- Interacting ω(q) dark energy model with phase space analysis (Q5067327) (← links)
- Hypersurface-Homogeneous Cosmological Models with Matter and Dark Energy (Q5069618) (← links)
- Whether dark energy can contribute to the treatment and healing of diseases (Q5237195) (← links)
