Forecasts on Interacting Dark Energy from 21-cm Angular Power Spectrum with BINGO and SKA observations
arXiv:2103.01796 · doi:10.1093/mnras/stab3256
Abstract
Neutral hydrogen (HI) intensity mapping is a promising technique to probe the large-scale structure of the Universe, improving our understanding on the late-time accelerated expansion. In this work, we first scrutinize how an alternative cosmology, interacting dark energy (IDE), can affect the 21-cm angular power spectrum relative to the concordance CDM model. We re-derive the 21-cm brightness temperature fluctuation in the context of such interaction and uncover an extra new contribution. Then we estimate the noise level of three upcoming HI intensity mapping surveys, BINGO, SKA1-MID Band1 and Band2, respectively, and employ a Fisher matrix approach to forecast their constraints on the IDE model. We find that while 2018 maintains its dominion over early-Universe parameter constraints, BINGO and SKA1-MID Band2 put complementary bounding to the latest CMB measurements on dark energy equation of state , the interacting strength and the reduced Hubble constant , and SKA1-MID Band1 even outperforms 2018 in these late-Universe parameter constraints. The expected minimum uncertainties are given by SKA1-MID Band1+: on , on , on HI bias , and an absolute uncertainty of about () on (). Moreover, we quantify the effects from systematics of the redshift bin number, redshift-space distortions, foreground residuals and uncertainties on the measured HI fraction, . Our results indicate a bright prospect for HI intensity mapping surveys in constraining IDE, whether on their own or further by synergies with other measurements.
20 pages, 13 figures, 9 tables, accepted for publication in MNRAS
References in corpus (26)
- The Kinematics of the Ultra-Faint Milky Way Satellites: Solving the Missing Satellite Problem
- Baryon Acoustic Oscillations in the Lyα forest of BOSS DR11 quasars
- The Five-Hundred-Meter Aperture Spherical Radio Telescope (FAST) Project
- Late-time cosmology with 21cm intensity mapping experiments
- On the (Non)Evolution of HI Disks over Cosmic Time
- Canadian Hydrogen Intensity Mapping Experiment (CHIME) Pathfinder
- Possibility of Precise Measurement of the Cosmological Power Spectrum With a Dedicated 21cm Survey After Reionization
- Stability of the curvature perturbation in dark sectors' mutual interacting models
- The Neutral Hydrogen Cosmological Mass Density at z=5
- HIRAX: A Probe of Dark Energy and Radio Transients
- Testing General Relativity with 21 cm intensity mapping
- The Tianlai project: a 21cm cosmology experiment
- Blind foreground subtraction for intensity mapping experiments
- Testing the interaction between dark energy and dark matter via latest observations
- The imprint of the interaction between dark sectors in large scale cosmic microwave background anisotropies
- Emulating the CFHTLenS Weak Lensing data: Cosmological Constraints from moments and Minkowski functionals
- Effects of dark sectors' mutual interaction on the growth of structures
- Searching for dark matter - dark energy interactions: going beyond the conformal case
- The BINGO Project I: Baryon Acoustic Oscillations from Integrated Neutral Gas Observations
- Theoretical and observational constraints on the HI intensity power spectrum
- Cosmological parameter forecasts for HI intensity mapping experiments using the angular power spectrum
- J-PAS: forecasts on interacting dark energy from baryon acoustic oscillations and redshift-space distortions
- Measuring the growth of structure with intensity mapping surveys
- Constraints on the dark matter and dark energy interactions from weak lensing bispectrum tomography
- The BINGO Project IV: Simulations for mission performance assessment and preliminary component separation steps
- Imprints of non-standard Dark Energy and Dark Matter Models on the 21cm Intensity Map Power Spectrum