PQCD analysis of atmospheric tau neutrino

Full metadata record

DC Field	Value	Language
dc.contributor.author	Yeh, TW	en_US
dc.date.accessioned	2014-12-08T15:26:15Z	-
dc.date.available	2014-12-08T15:26:15Z	-
dc.date.issued	2003	en_US
dc.identifier.isbn	981-238-284-4	en_US
dc.identifier.uri	http://hdl.handle.net/11536/18638	-
dc.description.abstract	We calculate the flux of v, produced in the atmosphere by cosmic ray-air collisions. The production channels of v, from the process pA -> X -> v(T)((v) over bar (T))Y with X = D-s W-+/-, Z, h(b), t (t) over bar, are considered. The calculations are performed by employing perturbative QCD (PQCD). The predicted v(T) flux phi v(T)(E) is given for energy range 10(3)GeV <= E <= 10(8)GeV.	en_US
dc.language.iso	en_US	en_US
dc.title	PQCD analysis of atmospheric tau neutrino	en_US
dc.type	Proceedings Paper	en_US
dc.identifier.journal	PROCEEDINGS OF THE 2002 INTERNATIONAL SYMPOSIUM ON COSMOLOGY AND PARTICLE ASTROPHYSICS	en_US
dc.citation.spage	191	en_US
dc.citation.epage	198	en_US
dc.contributor.department	物理研究所	zh_TW
dc.contributor.department	Institute of Physics	en_US
dc.identifier.wosnumber	WOS:000229639400015	-
Appears in Collections:	Conferences Paper