Cosmology with the Square Kilometre Array
We argue that the Square Kilometre Array has the potential to make both redshift (HI) surveys and radio continuum surveys that will revolutionize cosmological studies, provided that it has sufficient instantaneous field-of-view that these surveys can cover a hemisphere in a timescale ~1 yr. Adopting...
| Main Authors: | , , , |
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| Format: | Journal article |
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2004
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| _version_ | 1797056541839327232 |
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| author | Blake, C Abdalla, F Bridle, S Rawlings, S |
| author_facet | Blake, C Abdalla, F Bridle, S Rawlings, S |
| author_sort | Blake, C |
| collection | OXFORD |
| description | We argue that the Square Kilometre Array has the potential to make both redshift (HI) surveys and radio continuum surveys that will revolutionize cosmological studies, provided that it has sufficient instantaneous field-of-view that these surveys can cover a hemisphere in a timescale ~1 yr. Adopting this assumption, we focus on two key experiments which will yield fundamental new measurements in cosmology, characterizing the properties of the mysterious dark energy which dominates the dynamics of today's Universe. Experiment I will map out ~10^9 HI galaxies to redshift z~1.5, providing the premier measurement of the clustering power spectrum of galaxies: accurately delineating the acoustic oscillations and the `turnover'. Experiment II will quantify the cosmic shear distortion of ~10^10 radio continuum sources, determining a precise power spectrum of the dark matter, and its growth as a function of cosmic epoch. We contrast the performance of the SKA in precision cosmology with that of other facilities which will, probably or possibly, be available on a similar timescale. We conclude that data from the SKA will yield transformational science as the direct result of four key features: (i) the immense cosmic volumes probed, exceeding future optical redshift surveys by more than an order of magnitude; (ii) well-controlled systematic effects such as the narrow `k-space window function' for Experiment I and the accurately-known `point-spread function' for Experiment II; (iii) the ability to measure with high precision large-scale modes in the clustering power spectra, for which nuisance effects such as non-linear structure growth, peculiar velocities and `galaxy bias' are minimised; and (iv) different degeneracies between key parameters to those which are inherent in the CMB. |
| first_indexed | 2024-03-06T19:24:07Z |
| format | Journal article |
| id | oxford-uuid:1b2223aa-7020-4ab9-aac5-282e6d4defe7 |
| institution | University of Oxford |
| last_indexed | 2024-03-06T19:24:07Z |
| publishDate | 2004 |
| record_format | dspace |
| spelling | oxford-uuid:1b2223aa-7020-4ab9-aac5-282e6d4defe72022-03-26T10:58:38ZCosmology with the Square Kilometre ArrayJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:1b2223aa-7020-4ab9-aac5-282e6d4defe7Symplectic Elements at Oxford2004Blake, CAbdalla, FBridle, SRawlings, SWe argue that the Square Kilometre Array has the potential to make both redshift (HI) surveys and radio continuum surveys that will revolutionize cosmological studies, provided that it has sufficient instantaneous field-of-view that these surveys can cover a hemisphere in a timescale ~1 yr. Adopting this assumption, we focus on two key experiments which will yield fundamental new measurements in cosmology, characterizing the properties of the mysterious dark energy which dominates the dynamics of today's Universe. Experiment I will map out ~10^9 HI galaxies to redshift z~1.5, providing the premier measurement of the clustering power spectrum of galaxies: accurately delineating the acoustic oscillations and the `turnover'. Experiment II will quantify the cosmic shear distortion of ~10^10 radio continuum sources, determining a precise power spectrum of the dark matter, and its growth as a function of cosmic epoch. We contrast the performance of the SKA in precision cosmology with that of other facilities which will, probably or possibly, be available on a similar timescale. We conclude that data from the SKA will yield transformational science as the direct result of four key features: (i) the immense cosmic volumes probed, exceeding future optical redshift surveys by more than an order of magnitude; (ii) well-controlled systematic effects such as the narrow `k-space window function' for Experiment I and the accurately-known `point-spread function' for Experiment II; (iii) the ability to measure with high precision large-scale modes in the clustering power spectra, for which nuisance effects such as non-linear structure growth, peculiar velocities and `galaxy bias' are minimised; and (iv) different degeneracies between key parameters to those which are inherent in the CMB. |
| spellingShingle | Blake, C Abdalla, F Bridle, S Rawlings, S Cosmology with the Square Kilometre Array |
| title | Cosmology with the Square Kilometre Array |
| title_full | Cosmology with the Square Kilometre Array |
| title_fullStr | Cosmology with the Square Kilometre Array |
| title_full_unstemmed | Cosmology with the Square Kilometre Array |
| title_short | Cosmology with the Square Kilometre Array |
| title_sort | cosmology with the square kilometre array |
| work_keys_str_mv | AT blakec cosmologywiththesquarekilometrearray AT abdallaf cosmologywiththesquarekilometrearray AT bridles cosmologywiththesquarekilometrearray AT rawlingss cosmologywiththesquarekilometrearray |