Published 2022 | Version v1
Journal article

Measurement of the low energy 25Mg(p,γ)26Al resonances

  • 1. China Institute of Atomic Energy, P. O. Box 275(10), Beijing 102413 (China)
  • 2. Key Laboratory of Beam Technology of Ministry of Education, College of Nuclear Science and Technology, Beijing Normal University, Beijing 100875 (China)
  • 3. College of Physics and Optoelectronic Engineering, Shenzhen University, Shenzhen 518060 (China)

Description

The cosmic 1.809 MeV γ-ray emitted by the radioactive nucleus 26Al in the Galaxy is one of the key observation targets of the γ-ray astronomy. The 26Al is mainly produced by the 25Mg(p,γ)26Al reaction in the stellar Mg-Al reaction cycle. At the astrophysical relevant temperatures, the reaction rates of 25Mg(p,γ)26Al are dominated by several narrow resonances at low energy. This work reports a measurement of the low energy 25Mg(p,γ)26Al resonances at Jinping Underground Nuclear Astrophysics experimental facility (JUNA) in the China Jinping Underground Laboratory (CJPL).

Availability note (English)

Available from https://www.epj-conferences.org/articles/epjconf/pdf/2022/04/epjconf_nic16th2022_08002.pdf; https://doaj.org/article/f079edffa4d84361a55b0b6724d42732

Additional details

Publishing Information

Journal Title
EPJ. Web of Conferences
Journal Volume
260
Journal Page Range
vp.
ISSN
2100-014X

Conference

Title
16. International Symposium on Nuclei in the Cosmos
Dates
21-25 Sep 2021
Place
Chengdu (China)