21 cm power spectrum in interacting cubic Galileon model
arXiv:2208.11560 · doi:10.1007/s12036-023-09976-2
Abstract
We show the detectability of interacting and non-interacting cubic Galileon models from the CDM model through the 21 cm power spectrum. We show that the interferometric observations like the upcoming SKA1-mid can detect both the interacting and the non-interacting cubic Galileon model from the CDM model depending on the parameter values.
13 pages, 4 figures, comments are welcome
References in corpus (26)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Dynamics of dark energy
- Multi-messenger Observations of a Binary Neutron Star Merger
- Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
- Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
- Covariant Galileon
- Dark Energy after GW170817: dead ends and the road ahead
- Imperfect Dark Energy from Kinetic Gravity Braiding
- Approaches to Understanding Cosmic Acceleration
- The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
- Late-time cosmology with 21cm intensity mapping experiments
- Galileon Cosmology
- Cosmic Acceleration and the Helicity-0 Graviton
- Possibility of Precise Measurement of the Cosmological Power Spectrum With a Dedicated 21cm Survey After Reionization
- Galileon Gravity in Light of ISW, CMB, BAO and data
- On using visibility correlations to probe the HI distribution from the dark ages to the present epoch I: Formalism and the expected signal
- Mapping the Cosmological Expansion
- Density perturbations in general modified gravitational theories
- Modified gravity a la Galileon: Late time cosmic acceleration and observational constraints
- The multi-frequency angular power spectrum of the epoch of reionization 21 cm signal
- Modeling the neutral hydrogen distribution in the post-reionization Universe: intensity mapping
- Dark energy beyond quintessence: Constraints from the swampland
- Cosmology of the selfaccelerating third order Galileon
- Cosmic expansion parametrization: Implication for curvature and tension
- Observed galaxy power spectrum in cubic Galileon model
- Probing Compensated Isocurvature with the 21-cm Signal during Cosmic Dawn