{"volume":432,"oa_version":"Published Version","issue":"4","year":"2013","abstract":[{"lang":"eng","text":"Structures in Warm Dark Matter (WDM) models are exponentially suppressed below a certain scale, characterized by the dark matter particle mass, mx. Since structures form hierarchically, the presence of collapsed objects at high-redshifts can set strong lower limits on mx. We place robust constraints on mx using recent results from the {\\it Swift} database of high-redshift gamma-ray bursts (GRBs). We parameterize the redshift evolution of the ratio between the cosmic GRB rate and star formation rate (SFR) as ∝(1+z)α, thereby allowing astrophysical uncertainties to partially mimic the cosmological suppression of structures in WDM models. Using a maximum likelihood estimator on two different z>4 GRB subsamples (including two bursts at z>8), we constrain mx≳1.6-1.8 keV at 95% C.L., when marginalized over a flat prior in α. We further estimate that 5 years of a SVOM-like mission would tighten these constraints to mx≳2.3 keV. Our results show that GRBs are a powerful probe of high-redshift structures, providing robust and competitive constraints on mx."}],"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","quality_controlled":"1","oa":1,"date_created":"2024-09-06T07:25:13Z","publication":"Monthly Notices of the Royal Astronomical Society","publisher":"Oxford University Press","main_file_link":[{"url":"https://doi.org/10.1093/mnras/stt674","open_access":"1"}],"article_processing_charge":"No","extern":"1","_id":"17646","page":"3218-3227","article_type":"original","author":[{"last_name":"de Souza","first_name":"R. S.","full_name":"de Souza, R. S."},{"last_name":"Mesinger","full_name":"Mesinger, A.","first_name":"A."},{"last_name":"Ferrara","first_name":"A.","full_name":"Ferrara, A."},{"full_name":"Haiman, Zoltán","first_name":"Zoltán","last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36"},{"last_name":"Perna","full_name":"Perna, R.","first_name":"R."},{"full_name":"Yoshida, N.","first_name":"N.","last_name":"Yoshida"}],"month":"05","language":[{"iso":"eng"}],"title":"Constraints on warm dark matter models from high-redshift long gamma-ray bursts","day":"09","intvolume":" 432","date_published":"2013-05-09T00:00:00Z","scopus_import":"1","status":"public","type":"journal_article","doi":"10.1093/mnras/stt674","date_updated":"2024-09-24T12:40:52Z","publication_status":"published","publication_identifier":{"issn":["0035-8711","1365-2966"]},"citation":{"mla":"de Souza, R. S., et al. “Constraints on Warm Dark Matter Models from High-Redshift Long Gamma-Ray Bursts.” Monthly Notices of the Royal Astronomical Society, vol. 432, no. 4, Oxford University Press, 2013, pp. 3218–27, doi:10.1093/mnras/stt674.","chicago":"Souza, R. S. de, A. Mesinger, A. Ferrara, Zoltán Haiman, R. Perna, and N. Yoshida. “Constraints on Warm Dark Matter Models from High-Redshift Long Gamma-Ray Bursts.” Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2013. https://doi.org/10.1093/mnras/stt674.","ama":"de Souza RS, Mesinger A, Ferrara A, Haiman Z, Perna R, Yoshida N. Constraints on warm dark matter models from high-redshift long gamma-ray bursts. Monthly Notices of the Royal Astronomical Society. 2013;432(4):3218-3227. doi:10.1093/mnras/stt674","ista":"de Souza RS, Mesinger A, Ferrara A, Haiman Z, Perna R, Yoshida N. 2013. Constraints on warm dark matter models from high-redshift long gamma-ray bursts. Monthly Notices of the Royal Astronomical Society. 432(4), 3218–3227.","ieee":"R. S. de Souza, A. Mesinger, A. Ferrara, Z. Haiman, R. Perna, and N. Yoshida, “Constraints on warm dark matter models from high-redshift long gamma-ray bursts,” Monthly Notices of the Royal Astronomical Society, vol. 432, no. 4. Oxford University Press, pp. 3218–3227, 2013.","short":"R.S. de Souza, A. Mesinger, A. Ferrara, Z. Haiman, R. Perna, N. Yoshida, Monthly Notices of the Royal Astronomical Society 432 (2013) 3218–3227.","apa":"de Souza, R. S., Mesinger, A., Ferrara, A., Haiman, Z., Perna, R., & Yoshida, N. (2013). Constraints on warm dark matter models from high-redshift long gamma-ray bursts. Monthly Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stt674"}}