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arXiv 1901.01966nucl-ex
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$^{20}$ Mg($βpγ$)$^{19}$ Ne衰变的多普勒展宽

Doppler Broadening in $^{20}$Mg($βpγ$)$^{19}$Ne Decay

Brent E. Glassman, David Pérez-Loureiro, Chris Wrede, Jacob Allen, Dan W. Bardayan, Michael B. Bennett, Kelly A. Chipps, Michael Febbraro, Moshe Friedman, Cathl… 展开作者

Brent E. Glassman, David Pérez-Loureiro, Chris Wrede, Jacob Allen, Dan W. Bardayan, Michael B. Bennett, Kelly A. Chipps, Michael Febbraro, Moshe Friedman, Cathleen Fry, Matt Hall, Oscar Hall, Sean N. Liddick, Patrick O'Malley, Wei Jia Ong, Steven D. Pain, Sarah Schwartz, Praveen Shidling, Harry Sims, Paul Thompson, Helin Zhang

摘要:

背景资料:I型X射线爆发中的$^{15}$ O($α,γ$)$^{19}$ Ne瓶颈反应是最需要实验约束的热核反应速率,以提高爆发光变曲线模拟的精度。一种确定该反应热核速率的建议技术采用$^{20}$ Mg($βpα$)$^{15}$ O衰变序列。目前已知,在4.03 MeV激发下的关键$^{15}$ O($α,γ$)$^{19}$ Ne共振被注入$^{20}$ Mg($βpγ$)$^{19}$ Ne中;然而,注入4.03 MeV状态的质子的能量尚不清楚。质子能量的知识将有助于未来的$^{20}$ Mg($βp α$)$^{15}$ O测量。目的:测定$^{19}$ Ne的4.03 MeV质子跃迁能量。方法:将$^{20}$ Mg的快束注入塑料闪烁体中,用于探测$β$颗粒。使用16个高纯度锗探测器来探测$βp$衰变后发射的$γ$射线。用Monte Carlo方法模拟了$^{19}$ Ne $γ$射线的多普勒展宽,并与实验数据进行了比较。结果如下:质子和供给4.03 MeV状态的$^{19}$ Ne之间的质心能量被测量为1.21 ${^{+0.25}_{-0.22}}$ MeV,对应于7.44 ${^{+0.25}_{-0.22}}$ MeV的$^{20}$ Na激发能量。测定了包括1615 keV能级在内的$^{19}$ Ne态的绝对馈电强度和$γ$ -衰变分支比.报道了一个新的从$^{19}$ Ne的1536 keV态到基态的$γ$衰变分支。$^{19}$ Ne中1507 keV态的寿命测量为4.3 ${^{+1.3}_{-1.1}}$ ps,解决了文献中的差异。澄清了已发表文献中对$^{20}$ Mg($βp$)衰变方案的误解。

英文摘要:

Background: The $^{15}$O($α,γ$)$^{19}$Ne bottleneck reaction in Type I x-ray bursts is the most important thermonuclear reaction rate to constrain experimentally, in order to improve the accuracy of burst light-curve simulations. A proposed technique to determine the thermonuclear rate of this reaction employs the $^{20}$Mg($βpα$)$^{15}$O decay sequence. The key $^{15}$O($α,γ$)$^{19}$Ne resonance at an excitation of 4.03 MeV is now known to be fed in $^{20}$Mg($βpγ$)$^{19}$Ne; however, the energies of the protons feeding the 4.03 MeV state are unknown. Knowledge of the proton energies will facilitate future $^{20}$Mg($βp α$)$^{15}$O measurements. Purpose: To determine the energy of the proton transition feeding the 4.03 MeV state in $^{19}$Ne. Method: A fast beam of $^{20}$Mg was implanted into a plastic scintillator, which was used to detect $β$ particles. 16 high purity germanium detectors were used to detect $γ$ rays emitted following $βp$ decay. A Monte Carlo method was used to simulate the Doppler broadening of $^{19}$Ne $γ$ rays and compare to the experimental data. Results: The center of mass energy between the proton and $^{19}$Ne, feeding the 4.03 MeV state, is measured to be 1.21${^{+0.25}_{-0.22}}$ MeV, corresponding to a $^{20}$Na excitation energy of 7.44${^{+0.25}_{-0.22}}$ MeV. Absolute feeding intensities and $γ$-decay branching ratios of $^{19}$Ne states were determined including the 1615 keV state. A new $γ$ decay branch from the 1536 keV state in $^{19}$Ne to the ground state is reported. The lifetime of the 1507 keV state in $^{19}$Ne is measured to be 4.3${^{+1.3}_{-1.1}}$ ps resolving discrepancies in the literature. Conflicting $^{20}$Mg($βp$) decay schemes in published literature are clarified.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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