{"type":"journal_article","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_number":"011302","date_published":"2005-06-30T00:00:00Z","citation":{"chicago":"Wang, Sheng, Zoltán Haiman, Wayne Hu, Justin Khoury, and Morgan May. “Weighing Neutrinos with Galaxy Cluster Surveys.” Physical Review Letters. American Physical Society, 2005. https://doi.org/10.1103/physrevlett.95.011302.","mla":"Wang, Sheng, et al. “Weighing Neutrinos with Galaxy Cluster Surveys.” Physical Review Letters, vol. 95, 011302, American Physical Society, 2005, doi:10.1103/physrevlett.95.011302.","ieee":"S. Wang, Z. Haiman, W. Hu, J. Khoury, and M. May, “Weighing neutrinos with galaxy cluster surveys,” Physical Review Letters, vol. 95. American Physical Society, 2005.","ista":"Wang S, Haiman Z, Hu W, Khoury J, May M. 2005. Weighing neutrinos with galaxy cluster surveys. Physical Review Letters. 95, 011302.","short":"S. Wang, Z. Haiman, W. Hu, J. Khoury, M. May, Physical Review Letters 95 (2005).","apa":"Wang, S., Haiman, Z., Hu, W., Khoury, J., & May, M. (2005). Weighing neutrinos with galaxy cluster surveys. Physical Review Letters. American Physical Society. https://doi.org/10.1103/physrevlett.95.011302","ama":"Wang S, Haiman Z, Hu W, Khoury J, May M. Weighing neutrinos with galaxy cluster surveys. Physical Review Letters. 2005;95. doi:10.1103/physrevlett.95.011302"},"publication_identifier":{"eissn":["1079-7114"],"issn":["0031-9007"]},"day":"30","article_processing_charge":"No","arxiv":1,"author":[{"first_name":"Sheng","full_name":"Wang, Sheng","last_name":"Wang"},{"id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","orcid":"0000-0003-3633-5403","full_name":"Haiman, Zoltán","first_name":"Zoltán","last_name":"Haiman"},{"last_name":"Hu","full_name":"Hu, Wayne","first_name":"Wayne"},{"last_name":"Khoury","full_name":"Khoury, Justin","first_name":"Justin"},{"first_name":"Morgan","full_name":"May, Morgan","last_name":"May"}],"oa_version":"Preprint","oa":1,"abstract":[{"lang":"eng","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."}],"language":[{"iso":"eng"}],"publication":"Physical Review Letters","volume":95,"status":"public","month":"06","doi":"10.1103/physrevlett.95.011302","year":"2005","article_type":"original","publication_status":"published","_id":"17810","OA_type":"green","main_file_link":[{"url":"https://doi.org/10.48550/arXiv.astro-ph/0505390","open_access":"1"}],"date_created":"2024-09-06T11:38:41Z","publisher":"American Physical Society","scopus_import":"1","date_updated":"2024-11-12T10:21:28Z","OA_place":"repository","extern":"1","external_id":{"arxiv":["astro-ph/0505390"]},"intvolume":" 95","quality_controlled":"1","title":"Weighing neutrinos with galaxy cluster surveys"}