Pages that link to "Item:Q1770118"
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The following pages link to Phantom cosmology with non-minimally coupled real scalar field (Q1770118):
Displaying 14 items.
- Non-minimal coupling of the phantom field and cosmic acceleration (Q613067) (← links)
- Scale factor dependent equation of state for curvature inspired dark energy, phantom barrier and late cosmic acceleration (Q712882) (← links)
- Phantom expansion with non-linear Schrödinger-type formulation of scalar field cosmology (Q848687) (← links)
- Holographic dark energy in induced gravity (Q884792) (← links)
- Spatial periodicity of galaxy number counts, CMB anisotropy, and SNIa Hubble diagram based on the universe accompanied by a non-minimally coupled scalar field (Q944520) (← links)
- Phantom appearance of non-phantom matter in Bianchi type-I cosmological model (Q1945621) (← links)
- Gravitational quasinormal modes of regular phantom black hole (Q2364309) (← links)
- Exorcising \(w < -1\) (Q2484467) (← links)
- Constructing phantom with a nonminimally coupled complex scalar field (Q2506052) (← links)
- Dark energy cosmology with a Rarita-Schwinger field (Q2506110) (← links)
- INFLATION IS PERHAPS THE GENERIC FEATURE OF PHANTOM FIELD, NOT THE BIG-RIP (Q3442776) (← links)
- LATE TIME ACCELERATION IN 3-BRANE BRANS–DICKE COSMOLOGY (Q3630917) (← links)
- UNIFIED PHANTOM COSMOLOGIES (Q5311681) (← links)
- Dark energy cosmology with spinor field (Q6069606) (← links)