TeV Diffuse Emission From the Inner Galaxy

Please use this identifier to cite or link to this item: http://lrc.quangbinhuni.edu.vn:8181/dspace/handle/DHQB_123456789/4107

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DC Field	Value	Language
dc.contributor.author	Amid, Nayerhoda	-
dc.contributor.author	Francisco Salesa, Greus	-
dc.contributor.author	abrina, Casanova	-
dc.date.accessioned	2018-09-13T08:06:02Z	-
dc.date.available	2018-09-13T08:06:02Z	-
dc.date.issued	2018	-
dc.identifier.uri	http://lrc.quangbinhuni.edu.vn:8181/dspace/handle/DHQB_123456789/4107	-
dc.description.abstract	The TeV diffuse emission from the Galactic plane is produced by multi TeV electrons and nuclei interacting with radiation fields and ambient gas, respectively. Measurements of the TeV diffuse emission help constrain CR origin and transport properties. We present a preliminary analysis of HAWC diffuse emission data from the inner Galaxy. The HAWC measurements will be used to constrain particle transport properties close to the Galaxy center correlating the HAWC maps with predictions of the DRAGON code.	en_US
dc.language.iso	en	en_US
dc.publisher	Switzerland	en_US
dc.subject	high energy astrophysics	en_US
dc.subject	inner galaxy	en_US
dc.subject	gamma rays	en_US
dc.subject	diffuse emission	en_US
dc.subject	cosmic rays	en_US
dc.subject	interstellar medium	en_US
dc.title	TeV Diffuse Emission From the Inner Galaxy	en_US
Appears in Collections:	Maps

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