cosmography for high redshifts
arXiv:2110.05434 · doi:10.3390/universe7110441
Abstract
In light of the statistical performance of cosmological observations, in this work we present the cosmography in gravity. In this scenario we found a cosmological viable standard case that allows to reduce the degeneracy between several models already proposed in the literature. Furthermore, we constrain this model using Pantheon SNeIa compilation, Cosmic Chronometers and a newly GRB calibrated data sample. We found that with an appropriate strategy for including the cosmographic parameter, we do produce a viable cosmology with our model within gravity.
16 pages, 3 figures. Version accepted in Universe
References in corpus (19)
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- Dark torsion as the cosmic speed-up
- Modified teleparallel gravity: inflation without inflaton
- Einstein's Other Gravity and the Acceleration of the Universe
- The trouble with
- Teleparallel Gravity: From Theory to Cosmology
- On Born-Infeld Gravity in Weitzenbock spacetime
- Cosmological perturbations in f(T) gravity
- Good and bad tetrads in f(T) gravity
- A parametric model for dark energy
- Noether Symmetry Approach in teleparallel cosmology
- Cosmological bouncing solutions in f(T,B) gravity
- Black Holes in Gravity: Exact and Perturbed Solutions
- Gravitoelectromagnetism, Solar System Test and Weak-Field Solutions in Gravity with Observational Constraints
- de Sitter and Scaling solutions in a higher-order modified teleparallel theory
- Towards a model-independent reconstruction approach for late-time Hubble data
- Variational Principles in Teleparallel Gravity Theories
- Neural networks and standard cosmography with newly calibrated high redshift GRB observations
- Calibration of gamma-ray bursts luminosity correlations using gravitational waves as standard sirens