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.
arXiv comment13 pages, 4 figures, comments are welcome
References in corpus (73)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Planck 2015 results. XIII. Cosmological parameters
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Dynamics of dark energy
- Modified Gravity and Cosmology
- f(R) theories
- Multi-messenger Observations of a Binary Neutron Star Merger
- Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
- 4D Gravity on a Brane in 5D Minkowski Space
- The Case for a Positive Cosmological Lambda-term
- Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution
- Quintessence, Cosmic Coincidence, and the Cosmological Constant
- Baryonic Features in the Matter Transfer Function
- Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
- The galileon as a local modification of gravity
- Generalized G-inflation: Inflation with the most general second-order field equations
- H0LiCOW XIII. A 2.4% measurement of from lensed quasars: tension between early and late-Universe probes
- Massive Gravity
- Covariant Galileon
- Dark Energy after GW170817: dead ends and the road ahead
- Everything You Always Wanted To Know About The Cosmological Constant Problem (But Were Afraid To Ask)
- Strong Interactions and Stability in the DGP Model
- Imperfect Dark Energy from Kinetic Gravity Braiding
- The Growth of HII Regions During Reionization
- Classical and Quantum Consistency of the DGP Model
- Cosmological Parameter Estimation Using 21 cm Radiation from the Epoch of Reionization
- Approaches to Understanding Cosmic Acceleration
- Measuring the cosmological constant with redshift surveys
- The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
- Late-time cosmology with 21cm intensity mapping experiments
- Cosmology with Phase 1 of the Square Kilometre Array; Red Book 2018: Technical specifications and performance forecasts
- Galileon Cosmology
- Cosmology of a covariant Galileon field
- On the de Sitter swampland criterion
- Cosmic Acceleration and the Helicity-0 Graviton
- Self-Accelerating Universe in Galileon Cosmology
- Cosmology of the Galileon from Massive Gravity
- 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
- Galileon gravity and its relevance to late time cosmic acceleration
- Mapping the Cosmological Expansion
- Nonlinear structure formation in the Cubic Galileon gravity model
- 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
- Cosmic expansion and growth histories in Galileon scalar-tensor models of dark energy
- Evolution of linear cosmological perturbations and its observational implications in Galileon-type modified gravity
- Galileons in the Sky
- Gravity in the Era of Equality: Towards solutions to the Hubble problem without fine-tuned initial conditions
- Fluctuations in 21cm Emission After Reionization
- Modeling the neutral hydrogen distribution in the post-reionization Universe: intensity mapping
- Constraining cosmology and ionization history with combined 21 cm power spectrum and global signal measurements
- The 21cm Power Spectrum After Reionization
- Dark energy beyond quintessence: Constraints from the swampland
- Cosmology of the selfaccelerating third order Galileon
- Light mass galileons: Cosmological dynamics, mass screening and observational constraints
- Matter bispectrum in cubic Galileon cosmologies
- Polarised foreground removal at low radio frequencies using rotation measure synthesis: uncovering the signature of hydrogen reionisation
- Constraining large scale HI bias using redshifted 21-cm signal from the post-reionization epoch
- Cosmic expansion parametrization: Implication for curvature and tension
- Probing the bispectrum at high redshifts using 21 cm HI observations
- Do Observations Favour Galileon Over Quintessence?
- On using large scale correlation of the Ly- forest and redshifted 21-cm signal to probe HI distribution during the post reionization era
- Observed galaxy power spectrum in cubic Galileon model
- Weak lensing probe of cubic Galileon model
- Probing Compensated Isocurvature with the 21-cm Signal during Cosmic Dawn
- A study on Cubic Galileon Gravity Using N-body Simulations
- Prospects of probing quintessence with HI 21-cm intensity mapping survey
- First and second order cosmological perturbations in light mass Galileon models
- The parameter space of Cubic Galileon models for cosmic acceleration
- Consistency of Cubic Galileon Cosmology: Model-Independent Bounds from Background Expansion and Perturbative Analyses