TeV Diffuse Emission From the Inner Galaxy

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 diffus...

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Tác giả chính: Amid, Nayerhoda, Francisco Salesa, Greus, abrina, Casanova
Ngôn ngữ:English
Năm xuất bản: Switzerland 2018
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Truy cập Trực tuyến:http://lrc.quangbinhuni.edu.vn:8181/dspace/handle/DHQB_123456789/4107
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recordtype dspace
spelling oai:localhost:DHQB_123456789-41072018-10-22T08:43:44Z TeV Diffuse Emission From the Inner Galaxy Amid, Nayerhoda Francisco Salesa, Greus abrina, Casanova high energy astrophysics inner galaxy gamma rays diffuse emission cosmic rays interstellar medium 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. 2018-09-13T08:06:02Z 2018-09-13T08:06:02Z 2018 http://lrc.quangbinhuni.edu.vn:8181/dspace/handle/DHQB_123456789/4107 en Switzerland
institution Trung tâm Học liệu Đại học Quảng Bình (Dspace)
collection Trung tâm Học liệu Đại học Quảng Bình (Dspace)
language English
topic high energy astrophysics
inner galaxy
gamma rays
diffuse emission
cosmic rays
interstellar medium
spellingShingle high energy astrophysics
inner galaxy
gamma rays
diffuse emission
cosmic rays
interstellar medium
Amid, Nayerhoda
Francisco Salesa, Greus
abrina, Casanova
TeV Diffuse Emission From the Inner Galaxy
description 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.
author Amid, Nayerhoda
Francisco Salesa, Greus
abrina, Casanova
author_facet Amid, Nayerhoda
Francisco Salesa, Greus
abrina, Casanova
author_sort Amid, Nayerhoda
title TeV Diffuse Emission From the Inner Galaxy
title_short TeV Diffuse Emission From the Inner Galaxy
title_full TeV Diffuse Emission From the Inner Galaxy
title_fullStr TeV Diffuse Emission From the Inner Galaxy
title_full_unstemmed TeV Diffuse Emission From the Inner Galaxy
title_sort tev diffuse emission from the inner galaxy
publisher Switzerland
publishDate 2018
url http://lrc.quangbinhuni.edu.vn:8181/dspace/handle/DHQB_123456789/4107
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