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

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DC Field	Value	Language
dc.contributor.author	Bagla, J.S.	-
dc.date.accessioned	2021-07-13T06:14:53Z	-
dc.date.available	2021-07-13T06:14:53Z	-
dc.date.issued	2011	-
dc.identifier.citation	Proceedings of the 29th Meeting of the Astronomical Society of India, held 23-25 February, 2011. ASI Conference Series, Vol. 3, p. 140	en_US
dc.identifier.uri	http://cdsads.u-strasbg.fr/full/2011ASInC...3Q.140B	-
dc.identifier.uri	http://hdl.handle.net/123456789/3698	-
dc.description.abstract	I 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.language.iso	en	en_US
dc.publisher	Proceedings of the 29th Meeting of the Astronomical Society of India	en_US
dc.subject	Hyperfine transition	en_US
dc.subject	Helium-3	en_US
dc.title	Hyperfine transition of Helium-3 as a probe of the high redshift universe	en_US
dc.type	Article	en_US
Appears in Collections:	Research Articles

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