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Title: Decay of the key 92-keV resonance in the 25Mg(p,γ) reaction to the ground and isomeric states of the cosmic γ-ray emitter 26Al

Abstract

The 92-keV resonance in the 25Mg(p,γ)26Al reaction plays a key role in the production of 26Al at astrophysical burning temperatures of ≈100 MK in the Mg-Al cycle. However, the state can decay to feed either the ground, 26gAl, or isomeric state, 26mAl. It is the ground state that is critical as the source of cosmic γ rays. It is therefore important to precisely determine the ground-state branching fraction f0 of this resonance. Here we report on the identification of four γ-ray transitions from the 92-keV resonance, and determine the spin of the state and its ground-state branching fraction f0 = 0.52(2)stat(6)syst. The f0 value is the most precise reported to date, and at the lower end of the range of previously adopted values, implying a lower production rate of 26gAl and its cosmic 1809-keV γ rays.

Authors:
ORCiD logo; ; ; ORCiD logo; ; ; ; ORCiD logo; ; ; ; ; ; ORCiD logo
Publication Date:
Research Org.:
University of North Carolina, Chapel Hill, NC (United States); Argonne National Laboratory (ANL), Argonne, IL (United States)
Sponsoring Org.:
USDOE Office of Science (SC), Nuclear Physics (NP); STFC; European Union's Horizon 2020; Academy of Finland; Austrian Science Fund (FWF); European Union - Horizon 2020 Research and Innovation Programme
OSTI Identifier:
1737722
Alternate Identifier(s):
OSTI ID: 1764027; OSTI ID: 1812740
Grant/Contract Number:  
AC02-06CH11357; FG02-97ER41033; FG02-97ER41041; FG02-94ER40834; ST/J00006X/1; 771036; 275389
Resource Type:
Published Article
Journal Name:
Physics Letters. B
Additional Journal Information:
Journal Name: Physics Letters. B Journal Volume: 813 Journal Issue: C; Journal ID: ISSN 0370-2693
Publisher:
Elsevier
Country of Publication:
Netherlands
Language:
English
Subject:
73 NUCLEAR PHYSICS AND RADIATION PHYSICS; Nuclear astrophysics; 26Al; γ spectroscopy; Cosmic γ rays

Citation Formats

Kankainen, A., Woods, P. J., Doherty, D. T., Albers, H. M., Albers, M., Ayangeakaa, A. D., Carpenter, M. P., Chiara, C. J., Harker, J. L., Janssens, R. V. F., Lederer-Woods, C., Seweryniak, D., Strieder, F., and Zhu, S. Decay of the key 92-keV resonance in the 25Mg(p,γ) reaction to the ground and isomeric states of the cosmic γ-ray emitter 26Al. Netherlands: N. p., 2021. Web. doi:10.1016/j.physletb.2020.136033.
Kankainen, A., Woods, P. J., Doherty, D. T., Albers, H. M., Albers, M., Ayangeakaa, A. D., Carpenter, M. P., Chiara, C. J., Harker, J. L., Janssens, R. V. F., Lederer-Woods, C., Seweryniak, D., Strieder, F., & Zhu, S. Decay of the key 92-keV resonance in the 25Mg(p,γ) reaction to the ground and isomeric states of the cosmic γ-ray emitter 26Al. Netherlands. https://doi.org/10.1016/j.physletb.2020.136033
Kankainen, A., Woods, P. J., Doherty, D. T., Albers, H. M., Albers, M., Ayangeakaa, A. D., Carpenter, M. P., Chiara, C. J., Harker, J. L., Janssens, R. V. F., Lederer-Woods, C., Seweryniak, D., Strieder, F., and Zhu, S. Mon . "Decay of the key 92-keV resonance in the 25Mg(p,γ) reaction to the ground and isomeric states of the cosmic γ-ray emitter 26Al". Netherlands. https://doi.org/10.1016/j.physletb.2020.136033.
@article{osti_1737722,
title = {Decay of the key 92-keV resonance in the 25Mg(p,γ) reaction to the ground and isomeric states of the cosmic γ-ray emitter 26Al},
author = {Kankainen, A. and Woods, P. J. and Doherty, D. T. and Albers, H. M. and Albers, M. and Ayangeakaa, A. D. and Carpenter, M. P. and Chiara, C. J. and Harker, J. L. and Janssens, R. V. F. and Lederer-Woods, C. and Seweryniak, D. and Strieder, F. and Zhu, S.},
abstractNote = {The 92-keV resonance in the 25Mg(p,γ)26Al reaction plays a key role in the production of 26Al at astrophysical burning temperatures of ≈100 MK in the Mg-Al cycle. However, the state can decay to feed either the ground, 26gAl, or isomeric state, 26mAl. It is the ground state that is critical as the source of cosmic γ rays. It is therefore important to precisely determine the ground-state branching fraction f0 of this resonance. Here we report on the identification of four γ-ray transitions from the 92-keV resonance, and determine the spin of the state and its ground-state branching fraction f0 = 0.52(2)stat(6)syst. The f0 value is the most precise reported to date, and at the lower end of the range of previously adopted values, implying a lower production rate of 26gAl and its cosmic 1809-keV γ rays.},
doi = {10.1016/j.physletb.2020.136033},
journal = {Physics Letters. B},
number = C,
volume = 813,
place = {Netherlands},
year = {Mon Feb 01 00:00:00 EST 2021},
month = {Mon Feb 01 00:00:00 EST 2021}
}

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