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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| Ngôn ngữ: | English |
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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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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 |
| _version_ |
1717292474915880960 |
| score |
9,463379 |