Revised decay properties of the key 93-keV resonance in the 25Mg(p,γ) reaction and its influence on the MgAl cycle in astrophysical environments
dc.contributor.author | Lotay, G. | |
dc.contributor.author | Doherty, D. T. | |
dc.contributor.author | Janssens, R. V. F. | |
dc.contributor.author | Seweryniak, D. | |
dc.contributor.author | Albers, H. M. | |
dc.contributor.author | Almaraz-Calderon, S. | |
dc.contributor.author | Carpenter, M. P. | |
dc.contributor.author | Champagne, A. E. | |
dc.contributor.author | Chiara, C. J. | |
dc.contributor.author | Hoffman, C. R. | |
dc.contributor.author | Iliadis, C. | |
dc.contributor.author | Kankainen, A. | |
dc.contributor.author | Lauritsen, T. | |
dc.contributor.author | Zhu, S. | |
dc.date.accessioned | 2022-06-22T11:44:48Z | |
dc.date.available | 2022-06-22T11:44:48Z | |
dc.date.issued | 2022 | |
dc.identifier.citation | Lotay, G., Doherty, D. T., Janssens, R. V. F., Seweryniak, D., Albers, H. M., Almaraz-Calderon, S., Carpenter, M. P., Champagne, A. E., Chiara, C. J., Hoffman, C. R., Iliadis, C., Kankainen, A., Lauritsen, T., & Zhu, S. (2022). Revised decay properties of the key 93-keV resonance in the 25Mg(p,γ) reaction and its influence on the MgAl cycle in astrophysical environments. <i>Physical Review C</i>, <i>105</i>(4), Article L042801. <a href="https://doi.org/10.1103/PhysRevC.105.L042801" target="_blank">https://doi.org/10.1103/PhysRevC.105.L042801</a> | |
dc.identifier.other | CONVID_147090236 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/81985 | |
dc.description.abstract | The γ-decay properties of an excited state in 26Al at 6398.3(8) keV have been reexamined using the 11B+16O fusion-evaporation reaction. This level represents a key 93.1(8)-keV resonance in the 25Mg+p system and its relative branching to the 26Al ground state, f0, has been determined to be 0.76±0.03 (stat.) ±0.10 (syst.). This is a significantly higher value than the most recent evaluation and implies a considerable increase in the production of cosmic γ rays from 26Al radioactivity. | en |
dc.format.mimetype | application/pdf | |
dc.language.iso | eng | |
dc.publisher | American Physical Society (APS) | |
dc.relation.ispartofseries | Physical Review C | |
dc.rights | In Copyright | |
dc.title | Revised decay properties of the key 93-keV resonance in the 25Mg(p,γ) reaction and its influence on the MgAl cycle in astrophysical environments | |
dc.type | article | |
dc.identifier.urn | URN:NBN:fi:jyu-202206223590 | |
dc.contributor.laitos | Fysiikan laitos | fi |
dc.contributor.laitos | Department of Physics | en |
dc.contributor.oppiaine | Kiihdytinlaboratorio | fi |
dc.contributor.oppiaine | Accelerator Laboratory | en |
dc.type.uri | http://purl.org/eprint/type/JournalArticle | |
dc.type.coar | http://purl.org/coar/resource_type/c_2df8fbb1 | |
dc.description.reviewstatus | peerReviewed | |
dc.relation.issn | 2469-9985 | |
dc.relation.numberinseries | 4 | |
dc.relation.volume | 105 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | © 2022 American Physical Society (APS) | |
dc.rights.accesslevel | openAccess | fi |
dc.subject.yso | astrofysiikka | |
dc.subject.yso | ydinfysiikka | |
dc.subject.yso | magnesium | |
dc.subject.yso | alumiini | |
dc.subject.yso | kosminen säteily | |
dc.subject.yso | gammasäteily | |
dc.format.content | fulltext | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p20188 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p14759 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p3518 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p19563 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p14258 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p14248 | |
dc.rights.url | http://rightsstatements.org/page/InC/1.0/?language=en | |
dc.relation.doi | 10.1103/PhysRevC.105.L042801 | |
jyx.fundinginformation | This work was supported by the US Department of Energy, Office of Science, Office of Nuclear Physics, under Contract No. DEAC02-06CH11357 and Grants No. DEFG02-94ER40834, No. DEFG02-97ER41041, and No. DEFG02-97ER41033. UK personnel were supported by the Science and Technologies Facilities Council (STFC). This research uses resources of ANL's ATLAS facility, which is a DOE Office of Science User facility. | |
dc.type.okm | A1 |