{"language":[{"iso":"eng"}],"day":"30","volume":95,"scopus_import":"1","date_created":"2024-09-06T11:38:41Z","quality_controlled":"1","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_type":"original","year":"2005","OA_type":"green","title":"Weighing neutrinos with galaxy cluster surveys","oa_version":"Preprint","publication_identifier":{"eissn":["1079-7114"],"issn":["0031-9007"]},"intvolume":"        95","article_number":"011302","oa":1,"status":"public","abstract":[{"text":"Large future galaxy cluster surveys, combined with cosmic microwave background observations, can achieve a high sensitivity to the masses of cosmologically important neutrinos. We show that a weak lensing selected sample of ≳100 000 clusters could tighten the current upper bound on the sum of masses of neutrino species by an order of magnitude, to a level of 0.03 eV. Since this statistical sensitivity is below the best existing lower limit on the mass of at least one neutrino species, a future detection is likely, provided that systematic errors can be controlled to a similar level.","lang":"eng"}],"publisher":"American Physical Society","doi":"10.1103/physrevlett.95.011302","publication_status":"published","OA_place":"repository","_id":"17810","publication":"Physical Review Letters","main_file_link":[{"url":"https://doi.org/10.48550/arXiv.astro-ph/0505390","open_access":"1"}],"author":[{"last_name":"Wang","full_name":"Wang, Sheng","first_name":"Sheng"},{"orcid":"0000-0003-3633-5403","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman","full_name":"Haiman, Zoltán","first_name":"Zoltán"},{"full_name":"Hu, Wayne","first_name":"Wayne","last_name":"Hu"},{"full_name":"Khoury, Justin","first_name":"Justin","last_name":"Khoury"},{"full_name":"May, Morgan","first_name":"Morgan","last_name":"May"}],"arxiv":1,"extern":"1","type":"journal_article","external_id":{"arxiv":["astro-ph/0505390"]},"month":"06","citation":{"chicago":"Wang, Sheng, Zoltán Haiman, Wayne Hu, Justin Khoury, and Morgan May. “Weighing Neutrinos with Galaxy Cluster Surveys.” <i>Physical Review Letters</i>. American Physical Society, 2005. <a href=\"https://doi.org/10.1103/physrevlett.95.011302\">https://doi.org/10.1103/physrevlett.95.011302</a>.","mla":"Wang, Sheng, et al. “Weighing Neutrinos with Galaxy Cluster Surveys.” <i>Physical Review Letters</i>, vol. 95, 011302, American Physical Society, 2005, doi:<a href=\"https://doi.org/10.1103/physrevlett.95.011302\">10.1103/physrevlett.95.011302</a>.","short":"S. Wang, Z. Haiman, W. Hu, J. Khoury, M. May, Physical Review Letters 95 (2005).","ista":"Wang S, Haiman Z, Hu W, Khoury J, May M. 2005. Weighing neutrinos with galaxy cluster surveys. Physical Review Letters. 95, 011302.","ama":"Wang S, Haiman Z, Hu W, Khoury J, May M. Weighing neutrinos with galaxy cluster surveys. <i>Physical Review Letters</i>. 2005;95. doi:<a href=\"https://doi.org/10.1103/physrevlett.95.011302\">10.1103/physrevlett.95.011302</a>","apa":"Wang, S., Haiman, Z., Hu, W., Khoury, J., &#38; May, M. (2005). Weighing neutrinos with galaxy cluster surveys. <i>Physical Review Letters</i>. American Physical Society. <a href=\"https://doi.org/10.1103/physrevlett.95.011302\">https://doi.org/10.1103/physrevlett.95.011302</a>","ieee":"S. Wang, Z. Haiman, W. Hu, J. Khoury, and M. May, “Weighing neutrinos with galaxy cluster surveys,” <i>Physical Review Letters</i>, vol. 95. American Physical Society, 2005."},"date_published":"2005-06-30T00:00:00Z","article_processing_charge":"No","date_updated":"2024-11-12T10:21:28Z"}