Shahina, R. J. deBoer, J. Gorres, R. Fang, M. Febbraro, R. Kelmar, M. Matney, K. Manukyan, J. T. Nattress, E. Robles, T. J. Ruland, T. T. King, A. Sanchez, R. S. Sidhu, E. Stech, M. Wiescher
{"title":"Strength measurement of the $E_α^{lab}$ = 830 keV resonance in $^{22}\\rm{Ne}(α,n)^{25}\\rm{Mg}$ reaction using a stilbene detector","authors":"Shahina, R. J. deBoer, J. Gorres, R. Fang, M. Febbraro, R. Kelmar, M. Matney, K. Manukyan, J. T. Nattress, E. Robles, T. J. Ruland, T. T. King, A. Sanchez, R. S. Sidhu, E. Stech, M. Wiescher","doi":"arxiv-2409.01393","DOIUrl":null,"url":null,"abstract":"The interplay between the $^{22}$Ne$(\\alpha,\\gamma)^{26}$Mg and the competing\n$^{22}$Ne$(\\alpha,n)^{25}$Mg reactions determines the efficiency of the latter\nas a neutron source at the temperatures of stellar helium burning. In both\ncases, the rates are dominated by the $\\alpha$-cluster resonance at 830 keV.\nThis resonance plays a particularly important role in determining the strength\nof the neutron flux for both the weak and main $s$-process as well as the\n$n$-process. Recent experimental studies based on transfer reactions suggest\nthat the neutron and $\\gamma$-ray strengths for this resonance are\napproximately equal. In this study, the $^{22}$Ne$(\\alpha,n)^{25}$Mg resonance\nstrength has been remeasured and found to be similar to the previous direct\nstudies. This reinforces an 830 keV resonance strength that is approximately a\nfactor of three larger for the $^{22}$Ne$(\\alpha,n)^{25}$Mg reaction than for\nthe $^{22}$Ne$(\\alpha,\\gamma)^{26}$Mg reaction.","PeriodicalId":501206,"journal":{"name":"arXiv - PHYS - Nuclear Experiment","volume":"6 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Nuclear Experiment","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.01393","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
The interplay between the $^{22}$Ne$(\alpha,\gamma)^{26}$Mg and the competing
$^{22}$Ne$(\alpha,n)^{25}$Mg reactions determines the efficiency of the latter
as a neutron source at the temperatures of stellar helium burning. In both
cases, the rates are dominated by the $\alpha$-cluster resonance at 830 keV.
This resonance plays a particularly important role in determining the strength
of the neutron flux for both the weak and main $s$-process as well as the
$n$-process. Recent experimental studies based on transfer reactions suggest
that the neutron and $\gamma$-ray strengths for this resonance are
approximately equal. In this study, the $^{22}$Ne$(\alpha,n)^{25}$Mg resonance
strength has been remeasured and found to be similar to the previous direct
studies. This reinforces an 830 keV resonance strength that is approximately a
factor of three larger for the $^{22}$Ne$(\alpha,n)^{25}$Mg reaction than for
the $^{22}$Ne$(\alpha,\gamma)^{26}$Mg reaction.