Hyperfine transition of Helium-3 as a probe of the high redshift universe

dc.contributor.authorBagla, J.S.
dc.date.accessioned2021-07-13T06:14:53Z
dc.date.available2021-07-13T06:14:53Z
dc.date.issued2011
dc.description.abstractI will describe salient properties of the hyperfine transition of singly ionised Helium-3. I will discuss results of simulation and analytical studies to make a case for use of this transition as a probe of the high redshift universe.en_US
dc.identifier.citationProceedings of the 29th Meeting of the Astronomical Society of India, held 23-25 February, 2011. ASI Conference Series, Vol. 3, p. 140en_US
dc.identifier.urihttp://cdsads.u-strasbg.fr/full/2011ASInC...3Q.140B
dc.identifier.urihttp://hdl.handle.net/123456789/3698
dc.language.isoenen_US
dc.publisherProceedings of the 29th Meeting of the Astronomical Society of Indiaen_US
dc.subjectHyperfine transitionen_US
dc.subjectHelium-3en_US
dc.titleHyperfine transition of Helium-3 as a probe of the high redshift universeen_US
dc.typeArticleen_US

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