The hyperfine transition of 3He+ as a probe of the intergalactic medium

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dc.creatorBagla, J. S.
dc.creatorLoeb, Abraham
dc.date2009-05-12
dc.date.accessioned2026-07-07T13:13:58Z
dc.date.available2026-07-07T13:13:58Z
dc.descriptionWe explore the prospects of using the hyperfine transition of 3He+ as a probe of the intergalactic medium. The emission signal from ionized regions during reionization is expected to be anti-correlated with 21cm maps. The predicted emission signal from Lyman-alpha blobs at lower redshifts is detectable with future radio observatories.
dc.description5 pages, 1 figure, submitted to MNRAS
dc.identifierhttps://arxiv.org/abs/0905.1698
dc.identifierhttp://arxiv.org/abs/0905.1698
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/230066
dc.subjectCosmology and Nongalactic Astrophysics
dc.titleThe hyperfine transition of 3He+ as a probe of the intergalactic medium
dc.typetext

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