Pages that link to "Item:Q2922970"
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The following pages link to Constraining chameleon models with cosmology (Q2922970):
Displaying 16 items.
- Constraining \(f(R)\) gravity in solar system, cosmology and binary pulsar systems (Q1738391) (← links)
- Modified gravity with disappearing cosmological constant (Q2085396) (← links)
- Beyond self-acceleration: force- and fluid-acceleration (Q2188718) (← links)
- A natural cosmological constant from chameleons (Q2399015) (← links)
- Tests of chameleon gravity (Q2632847) (← links)
- Effects of chameleon scalar field on rotation curves of the galaxies (Q2865276) (← links)
- Cosmological probes of modified gravity: the nonlinear regime (Q2889153) (← links)
- CHAMELEON COSMOLOGY MODEL DESCRIBING THE PHANTOM DIVIDE LINE CROSSING (Q3019443) (← links)
- Parameterised post-Newtonian expansion in screened regions (Q5021840) (← links)
- Splashback in galaxy clusters as a probe of cosmic expansion and gravity (Q5023704) (← links)
- Speeding up<i>N</i>-body simulations of modified gravity: chameleon screening models (Q5024152) (← links)
- Constraints on the distance duality relation with standard sirens (Q5027079) (← links)
- Parameterised post-Newtonian formalism for the effective field theory of dark energy via screened reconstructed Horndeski theories (Q5027095) (← links)
- Hybrid <i>P</i><sub>ℓ</sub>(<i>k</i>): general, unified, non-linear matter power spectrum in redshift space (Q5070926) (← links)
- Chameleon screening depends on the shape and structure of NFW halos (Q5099263) (← links)
- Phenomenological footprints of Λ varying gravity theories inspired from quantum gravity models in the multi-messenger era (Q6074461) (← links)
