Cosmography in gravity
arXiv:2011.00420 · doi:10.1103/PhysRevD.102.124029
Abstract
Cosmography is an ideal tool to investigate the cosmic expansion history of the Universe in a model-independent way. The equations of motion in modified theories of gravity are usually very complicated; cosmography may select practical models without imposing arbitrary choices a priori. We use the model-independent way to derive and its derivatives up to fourth order in terms of measurable cosmographic parameters. We then fit those functions into the luminosity distance directly. We perform the MCMC analysis by considering three different sets of cosmographic functions. Using the largest supernovae Ia Pantheon sample, we derive the constraints on the Hubble constant and the cosmographic functions, and find that the former two terms in Taylor expansion of luminosity distance work dominantly in gravity.
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- Late-time cosmology with phantom dark-energy in gravity
- Constraining effective equation of state in gravity
- Cosmological bouncing scenarios in symmetric teleparallel gravity
- Accelerating Universe scenario in anisotropic cosmology
- A study of anisotropic spheres in gravity with quintessence field
- Power-law cosmology in Weyl-type gravity
- Transit String Dark Energy Models in Gravity
- Bulk viscous fluid in extended symmetric teleparallel gravity
- gravity, its covariant formulation, energy conservation and phase-space analysis
- Barrow holographic dark energy models in symmetric teleparallel gravity with Lambert function distribution
- Quantum Cosmology in theory
- Metric-Affine Myrzakulov Gravity Theories