[{"issue":"6","external_id":{"arxiv":["0306053"]},"intvolume":"        68","_id":"17759","status":"public","oa_version":"Preprint","day":"29","arxiv":1,"publisher":"American Physical Society","citation":{"ista":"Hu W, Haiman Z. 2003. Redshifting rings of power. Physical Review D. 68(6), 063004.","ama":"Hu W, Haiman Z. Redshifting rings of power. <i>Physical Review D</i>. 2003;68(6). doi:<a href=\"https://doi.org/10.1103/physrevd.68.063004\">10.1103/physrevd.68.063004</a>","apa":"Hu, W., &#38; Haiman, Z. (2003). Redshifting rings of power. <i>Physical Review D</i>. American Physical Society. <a href=\"https://doi.org/10.1103/physrevd.68.063004\">https://doi.org/10.1103/physrevd.68.063004</a>","ieee":"W. Hu and Z. Haiman, “Redshifting rings of power,” <i>Physical Review D</i>, vol. 68, no. 6. American Physical Society, 2003.","chicago":"Hu, Wayne, and Zoltán Haiman. “Redshifting Rings of Power.” <i>Physical Review D</i>. American Physical Society, 2003. <a href=\"https://doi.org/10.1103/physrevd.68.063004\">https://doi.org/10.1103/physrevd.68.063004</a>.","short":"W. Hu, Z. Haiman, Physical Review D 68 (2003).","mla":"Hu, Wayne, and Zoltán Haiman. “Redshifting Rings of Power.” <i>Physical Review D</i>, vol. 68, no. 6, 063004, American Physical Society, 2003, doi:<a href=\"https://doi.org/10.1103/physrevd.68.063004\">10.1103/physrevd.68.063004</a>."},"year":"2003","date_published":"2003-09-29T00:00:00Z","article_type":"original","fulldoi":"https://doi.org/10.1103/physrevd.68.063004","date_updated":"2024-09-30T08:47:45Z","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","abstract":[{"text":"The cosmic microwave background (CMB) has provided a precise template for features in the linear power spectrum: the matter-radiation turnover, sound horizon drop, and acoustic oscillations. In a two-dimensional power spectrum in redshift and angular space, the features appear as distorted rings, and yield simultaneous, purely geometric, measures of the Hubble parameter 𝐻⁡(𝑧) and angular diameter distance 𝐷𝐴⁡(𝑧) via an absolute version of the Alcock-Paczynski test. Employing a simple Fisher matrix tool, we explore how future surveys can exploit these rings of power for dark energy studies. High-z CMB determinations of H and 𝐷𝐴 are best complemented at moderate to low redshift (𝑧≲0.5) with a population of objects that are at least as abundant as clusters of galaxies. We find that a sample similar to that of the ongoing SDSS luminous red galaxy survey can achieve statistical errors at the ∼5% level for 𝐷𝐴⁡(𝑧) and 𝐻⁡(𝑧) in several redshift bins. This, in turn, implies errors of 𝜎⁡(𝑤)=0.03–0.05 for a constant dark energy equation of state in a flat universe. Deep galaxy cluster surveys such as the planned South Pole Telescope survey can extend this test out to 𝑧∼1 or as far as redshift follow-up is available. We find that the expected constraints are at the 𝜎⁡(𝑤)=0.04–0.08 level, comparable to those of galaxies and complementary in redshift coverage.","lang":"eng"}],"article_processing_charge":"No","date_created":"2024-09-06T09:46:11Z","quality_controlled":"1","publication_status":"published","volume":68,"language":[{"iso":"eng"}],"month":"09","title":"Redshifting rings of power","oa":1,"publication_identifier":{"issn":["0556-2821","1089-4918"]},"type":"journal_article","main_file_link":[{"url":" https://doi.org/10.48550/arXiv.astro-ph/0306053","open_access":"1"}],"doi":"10.1103/physrevd.68.063004","article_number":"063004","extern":"1","scopus_import":"1","publication":"Physical Review D","author":[{"last_name":"Hu","full_name":"Hu, Wayne","first_name":"Wayne"},{"last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","full_name":"Haiman, Zoltán","first_name":"Zoltán"}]}]