The high-energy galactic tau neutrino flux and its atmospheric background

完整後設資料紀錄

DC 欄位	值	語言
dc.contributor.author	Athar, Husain	en_US
dc.contributor.author	Cheung, Kingman	en_US
dc.contributor.author	Lin, Guey-Lin	en_US
dc.contributor.author	Tseng, Jie-Jun	en_US
dc.date.accessioned	2014-12-08T15:38:51Z	-
dc.date.available	2014-12-08T15:38:51Z	-
dc.date.issued	2004-07-01	en_US
dc.identifier.issn	1434-6044	en_US
dc.identifier.uri	http://dx.doi.org/10.1140/epjcd/s2004-03-1844-9	en_US
dc.identifier.uri	http://hdl.handle.net/11536/26606	-
dc.description.abstract	We compare the tau neutrino flux arising from the galaxy and the earth atmosphere for 10(3) <= E/GeV <= 10(11). The intrinsic and oscillated tau neutrino fluxes from both sources are considered. We find that, for E >= 10(3) GeV, the oscillated nu(tau) flux along the galactic plane dominates over the maximal intrinsic atmospheric nu(tau) flux, i.e., the flux along the horizontal direction. We also briefly comment on the prospects for observing these high-energy tau neutrinos.	en_US
dc.language.iso	en_US	en_US
dc.title	The high-energy galactic tau neutrino flux and its atmospheric background	en_US
dc.type	Article	en_US
dc.identifier.doi	10.1140/epjcd/s2004-03-1844-9	en_US
dc.identifier.journal	EUROPEAN PHYSICAL JOURNAL C	en_US
dc.citation.volume	33	en_US
dc.citation.issue		en_US
dc.citation.spage	S959	en_US
dc.citation.epage	S961	en_US
dc.contributor.department	物理研究所	zh_TW
dc.contributor.department	Institute of Physics	en_US
dc.identifier.wosnumber	WOS:000207563000260	-
dc.citation.woscount	2	-
顯示於類別：	期刊論文

文件中的檔案：

若為 zip 檔案，請下載檔案解壓縮後，用瀏覽器開啟資料夾中的 index.html 瀏覽全文。