Forecasts of cosmological constraints from HI intensity mapping with FAST, BINGO and SKA-I
Creators
- 1. Astrophysics and Cosmology Research Unit, School of Mathematics, Statistics and Computer Science, University of KwaZulu-Natal,Westville Campus, Private Bag X54001, Durban, 4000 (South Africa)
- 2. Astrophysics and Cosmology Research Unit, School of Chemistry and Physics, University of KwaZulu-Natal, Westville Campus, Private Bag X54001, Durban, 4000 (South Africa)
Description
We forecast the cosmological constraints of the neutral hydrogen (Hi) intensity mapping (IM) technique with radio telescopes by assuming 1-year of observational time. The current and future radio telescopes that we consider here are Five-hundred-meter Aperture Spherical radio Telescope (FAST), Baryon acoustic oscillations In Neutral Gas Observations (BINGO), and Square Kilometre Array phase I (SKA-I) single-dish experiments. We also forecast the combined constraints of the three radio telescopes with Planck. We find that the 1σ errors of (w 0, wa) for BINGO, FAST and SKA-I with respect to the fiducial values are respectively, (0.9293, 3.5792), (0.4083, 1.5878) and (0.3158, 0.4622). This is equivalent to (56.04%, 55.64%) and (66.02%, 87.09%) improvements in constraining (w 0, wa) for FAST and SKA-I respectively relative to BINGO. Simulations further show that SKA-I will put more stringent constraints than both FAST and BINGO when each of the experiments is combined with Planck measurements. The 1σ errors for (w 0, wa), BINGO + Planck, FAST + Planck and SKA-I + Planck covariance matrices are respectively (0.0832, 0.3520), (0.0791, 0.3313) and (0.0678, 0.2679) implying there is an improvement in (w 0, wa) constraints of (4.93%, 5.88%) for FAST + Planck relative to BINGO + Planck and an improvement of (18.51%, 23.89%) in constraining (w 0, wa) for SKA-I + Planck relative to BINGO + Planck. We also compared the performance of Planck data plus each single-dish experiment relative to Planck alone, and find that the reduction in (w 0, wa) 1σ errors for each experiment plus Planck, respectively, imply the (w 0, wa) constraints improvement of (22.96%, 8.45%), (26.76%, 13.84%) and (37.22%, 30.33%) for BINGO + Planck, FAST + Planck and SKA-I + Planck relative to Planck alone. For the nine cosmological parameters in consideration, we find that there is a trade-off between SKA-I and FAST in constraining cosmological parameters, with each experiment being more superior in constraining a particular set of parameters. (paper)
Availability note (English)
Available from http://dx.doi.org/10.1088/1674-4527/19/12/186Additional details
Identifiers
Publishing Information
- Journal Title
- Research in Astronomy and Astrophysics
- Journal Volume
- 19
- Journal Issue
- 12
- Journal Page Range
- [18 p.]
- ISSN
- 1674-4527
INIS
- Country of Publication
- China
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 51068101
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BARYONS; COMPARATIVE EVALUATIONS; COMPUTERIZED SIMULATION; H1 REGIONS; HYDROGEN; OSCILLATIONS; RADIO TELESCOPES
- Descriptors DEC
- ANTENNAS; COSMIC RADIO SOURCES; ELECTRICAL EQUIPMENT; ELECTRONIC EQUIPMENT; ELEMENTARY PARTICLES; ELEMENTS; EQUIPMENT; EVALUATION; FERMIONS; HADRONS; NONMETALS; RADIO EQUIPMENT; SIMULATION; TELESCOPES