Measurement of the low energy 25 Mg( p , γ ) 26 Al resonances
The cosmic 1.809 MeV γ -ray emitted by the radioactive nucleus 26 Al in the Galaxy is one of the key observation targets of the γ-ray astronomy. The 26 Al is mainly produced by the 25 Mg(p, γ ) 26 Al reaction in the stellar Mg-Al reaction cycle. At the astrophysical relevant temperatures, the reacti...
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creator | Su, Jun Li, Zhihong Zhang, Hao Li, Yunju Li, Ertao Chen, Chen Shen, Yangping He, Jianjun Zhang, Liyong Li, Xinyue Lian, Gang Guo, Bing Wang, Luohuan Sheng, Yaode Chen, Yinji Zhang, Long Cao, Fuqiang Liu, Weiping |
description | The cosmic 1.809 MeV
γ
-ray emitted by the radioactive nucleus
26
Al in the Galaxy is one of the key observation targets of the γ-ray astronomy. The
26
Al is mainly produced by the
25
Mg(p,
γ
)
26
Al reaction in the stellar Mg-Al reaction cycle. At the astrophysical relevant temperatures, the reaction rates of
25
Mg(p,
γ
)
26
Al are dominated by several narrow resonances at low energy. This work reports a measurement of the low energy
25
Mg(p,
γ
)
26
Al resonances at Jinping Underground Nuclear Astrophysics experimental facility (JUNA) in the China Jinping Underground Laboratory (CJPL). |
doi_str_mv | 10.1051/epjconf/202226008002 |
format | Article |
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γ
-ray emitted by the radioactive nucleus
26
Al in the Galaxy is one of the key observation targets of the γ-ray astronomy. The
26
Al is mainly produced by the
25
Mg(p,
γ
)
26
Al reaction in the stellar Mg-Al reaction cycle. At the astrophysical relevant temperatures, the reaction rates of
25
Mg(p,
γ
)
26
Al are dominated by several narrow resonances at low energy. This work reports a measurement of the low energy
25
Mg(p,
γ
)
26
Al resonances at Jinping Underground Nuclear Astrophysics experimental facility (JUNA) in the China Jinping Underground Laboratory (CJPL).</description><identifier>ISSN: 2100-014X</identifier><identifier>EISSN: 2100-014X</identifier><identifier>DOI: 10.1051/epjconf/202226008002</identifier><language>eng</language><ispartof>EPJ Web of conferences, 2022, Vol.260, p.8002</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-crossref_primary_10_1051_epjconf_2022260080023</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,860,4010,27900,27901,27902</link.rule.ids></links><search><creatorcontrib>Su, Jun</creatorcontrib><creatorcontrib>Li, Zhihong</creatorcontrib><creatorcontrib>Zhang, Hao</creatorcontrib><creatorcontrib>Li, Yunju</creatorcontrib><creatorcontrib>Li, Ertao</creatorcontrib><creatorcontrib>Chen, Chen</creatorcontrib><creatorcontrib>Shen, Yangping</creatorcontrib><creatorcontrib>He, Jianjun</creatorcontrib><creatorcontrib>Zhang, Liyong</creatorcontrib><creatorcontrib>Li, Xinyue</creatorcontrib><creatorcontrib>Lian, Gang</creatorcontrib><creatorcontrib>Guo, Bing</creatorcontrib><creatorcontrib>Wang, Luohuan</creatorcontrib><creatorcontrib>Sheng, Yaode</creatorcontrib><creatorcontrib>Chen, Yinji</creatorcontrib><creatorcontrib>Zhang, Long</creatorcontrib><creatorcontrib>Cao, Fuqiang</creatorcontrib><creatorcontrib>Liu, Weiping</creatorcontrib><title>Measurement of the low energy 25 Mg( p , γ ) 26 Al resonances</title><title>EPJ Web of conferences</title><description>The cosmic 1.809 MeV
γ
-ray emitted by the radioactive nucleus
26
Al in the Galaxy is one of the key observation targets of the γ-ray astronomy. The
26
Al is mainly produced by the
25
Mg(p,
γ
)
26
Al reaction in the stellar Mg-Al reaction cycle. At the astrophysical relevant temperatures, the reaction rates of
25
Mg(p,
γ
)
26
Al are dominated by several narrow resonances at low energy. This work reports a measurement of the low energy
25
Mg(p,
γ
)
26
Al resonances at Jinping Underground Nuclear Astrophysics experimental facility (JUNA) in the China Jinping Underground Laboratory (CJPL).</description><issn>2100-014X</issn><issn>2100-014X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><recordid>eNqdzj0KwkAQBeBFFAyaG1hMqaBmdvKDaQQRxcbOwm4JYRINyW7YVcRzeQ_PpIKFta95r3nwCTGSOJcYy4DbKje6CAiJKEFcIFJHeCQRZyijY_dn94XvXIXvhGkaxoknlnvO3NVyw_oCpoDLiaE2N2DNtrwDxbAvx9DCFJ4PmAAlsKrBsjM60zm7oegVWe3Y__ZARNvNYb2b5dY4Z7lQrT03mb0rierDVV-u-uWGf95eJm1JFw</recordid><startdate>2022</startdate><enddate>2022</enddate><creator>Su, Jun</creator><creator>Li, Zhihong</creator><creator>Zhang, Hao</creator><creator>Li, Yunju</creator><creator>Li, Ertao</creator><creator>Chen, Chen</creator><creator>Shen, Yangping</creator><creator>He, Jianjun</creator><creator>Zhang, Liyong</creator><creator>Li, Xinyue</creator><creator>Lian, Gang</creator><creator>Guo, Bing</creator><creator>Wang, Luohuan</creator><creator>Sheng, Yaode</creator><creator>Chen, Yinji</creator><creator>Zhang, Long</creator><creator>Cao, Fuqiang</creator><creator>Liu, Weiping</creator><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>2022</creationdate><title>Measurement of the low energy 25 Mg( p , γ ) 26 Al resonances</title><author>Su, Jun ; Li, Zhihong ; Zhang, Hao ; Li, Yunju ; Li, Ertao ; Chen, Chen ; Shen, Yangping ; He, Jianjun ; Zhang, Liyong ; Li, Xinyue ; Lian, Gang ; Guo, Bing ; Wang, Luohuan ; Sheng, Yaode ; Chen, Yinji ; Zhang, Long ; Cao, Fuqiang ; Liu, Weiping</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-crossref_primary_10_1051_epjconf_2022260080023</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Su, Jun</creatorcontrib><creatorcontrib>Li, Zhihong</creatorcontrib><creatorcontrib>Zhang, Hao</creatorcontrib><creatorcontrib>Li, Yunju</creatorcontrib><creatorcontrib>Li, Ertao</creatorcontrib><creatorcontrib>Chen, Chen</creatorcontrib><creatorcontrib>Shen, Yangping</creatorcontrib><creatorcontrib>He, Jianjun</creatorcontrib><creatorcontrib>Zhang, Liyong</creatorcontrib><creatorcontrib>Li, Xinyue</creatorcontrib><creatorcontrib>Lian, Gang</creatorcontrib><creatorcontrib>Guo, Bing</creatorcontrib><creatorcontrib>Wang, Luohuan</creatorcontrib><creatorcontrib>Sheng, Yaode</creatorcontrib><creatorcontrib>Chen, Yinji</creatorcontrib><creatorcontrib>Zhang, Long</creatorcontrib><creatorcontrib>Cao, Fuqiang</creatorcontrib><creatorcontrib>Liu, Weiping</creatorcontrib><collection>CrossRef</collection><jtitle>EPJ Web of conferences</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Su, Jun</au><au>Li, Zhihong</au><au>Zhang, Hao</au><au>Li, Yunju</au><au>Li, Ertao</au><au>Chen, Chen</au><au>Shen, Yangping</au><au>He, Jianjun</au><au>Zhang, Liyong</au><au>Li, Xinyue</au><au>Lian, Gang</au><au>Guo, Bing</au><au>Wang, Luohuan</au><au>Sheng, Yaode</au><au>Chen, Yinji</au><au>Zhang, Long</au><au>Cao, Fuqiang</au><au>Liu, Weiping</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Measurement of the low energy 25 Mg( p , γ ) 26 Al resonances</atitle><jtitle>EPJ Web of conferences</jtitle><date>2022</date><risdate>2022</risdate><volume>260</volume><spage>8002</spage><pages>8002-</pages><issn>2100-014X</issn><eissn>2100-014X</eissn><abstract>The cosmic 1.809 MeV
γ
-ray emitted by the radioactive nucleus
26
Al in the Galaxy is one of the key observation targets of the γ-ray astronomy. The
26
Al is mainly produced by the
25
Mg(p,
γ
)
26
Al reaction in the stellar Mg-Al reaction cycle. At the astrophysical relevant temperatures, the reaction rates of
25
Mg(p,
γ
)
26
Al are dominated by several narrow resonances at low energy. This work reports a measurement of the low energy
25
Mg(p,
γ
)
26
Al resonances at Jinping Underground Nuclear Astrophysics experimental facility (JUNA) in the China Jinping Underground Laboratory (CJPL).</abstract><doi>10.1051/epjconf/202226008002</doi></addata></record> |
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title | Measurement of the low energy 25 Mg( p , γ ) 26 Al resonances |
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