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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Veröffentlicht in:EPJ Web of conferences 2022, Vol.260, p.8002
Hauptverfasser: 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
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container_title EPJ Web of conferences
container_volume 260
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).
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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. 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title Measurement of the low energy 25 Mg( p , γ ) 26 Al resonances
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