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A unique set of transition matrix elements for the deuterium(vector deuteron,photon) 4-helium reaction at E(beam) = keV.

机译:一组独特的过渡矩阵元素,用于在E(beam)= keV的氘(矢量氘,光子)4-氦反应。

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The synthesis of the light elements in the first thousand seconds of the evolution of the Universe can be used to test the standard cosmology. Big-Bang Nucleosynthesis (BBN) is the only observational test of the hot big-bang model at early times, and the comparison between the calculated and observed abundances of 2H, 3He, 4He, and 7Li can be used to constrain the predicted baryon density of the Universe as well as the number of species of light particles. To reliably calculate the light element abundances it is necessary to reduce uncertainties in the BBN network reaction rates. The deuteron-deuteron radiative capture reaction is one of the deuterium-burning processes for which the cross section is not known well at very low energies (10–100 keV). Polarized beams allow accurate extraction of the complex transition matrix elements (TMEs) from the measured analyzing powers, such studies of the reaction mechanisms should lead to a reliable extrapolation of the cross section to energies relevant to BBN.; Prior to any polarized beam measurements, the 2H(d,γ) 4He reaction was believed to proceed entirely via electric quadrupole (E2) radiation at very low energies, a result of s-wave (angular momentum of the two deuterons l = 0) capture. However, low-energy measurements of 2H( d&ar; ,γ)4He analyzing powers revealed the presence of non-E2 radiation, appearing because of the presence of other than s-wave capture terms. Those studies showed that 50 to 85% of the total capture strength is due to p-wave (l = 1) capture. Unfortunately, the data analysis did not allow an unambiguous set of TMEs to be extracted, so that a critical test of theoretical results could not be performed.; In my work we were able to reduce uncertainties and expand the angular range in the measurements of the polarization observables. We obtained angular distributions for vector and tensor analyzing powers Ay and T20 by stopping a polarized deuteron beam of E d(lab) = 115 keV in a heavy-water ice target. The analysis of the data included l = 1 partial waves in addition to the s-wave (E2) capture term, corresponding to electric dipole (E1) and magnetic quadrupole (M2) radiation. A unique fit was obtained with an s-wave (E2) capture strength of 55 ± 8% of the total strength, and a p-wave strength of 29 ± 6% (E1) and 16 ± 3% (M2), for a total of 45 ± 7%. The measured analyzing powers and the results of the TME analysis were compared to refined resonating-group-model calculations. The observed and the calculated transition amplitudes were found to be in good agreement, although the p-wave phases disagree with the experimentally determined results, which will require further comparison of our analysis with the calculation.; Finally, the p-wave strength established by this work leads to the extrapolated value of the astrophysical S-factor for the 2H( d&ar; ,γ)4He reaction of 2 times lower than the previous best calculation.
机译:在宇宙演化的最初一千秒内,光元素的合成可用于测试标准宇宙学。大爆炸核合成(BBN)是热大爆炸模型在早期的唯一观测测试,并且计算的和观察到的 2 H, 3 He, 4 He和 7 Li可用于约束预测的宇宙重子密度以及轻粒子的种类数。为了可靠地计算轻元素的丰度,必须减少BBN网络反应速率的不确定性。氘-氘辐射捕获反应是氘燃烧过程之一,在非常低的能量(10-100 keV)下,其横截面并不为人所知。偏振光束可以从测得的分析能力中准确提取出复杂的过渡矩阵元素(TME),对反应机理的此类研究应能将横截面可靠地外推至​​与BBN相关的能量。在进行任何极化光束测量之前,人们认为 2 H(d,γ) 4 He反应完全是通过四极电子(E2)辐射以非常低的能量进行的, s波捕获结果(两个氘代 l 的角动量= 0)。但是, 2 H( d &ar; ,γ) 4 他的分析能力揭示了非E2辐射的存在,这是由于存在非s波捕获项而出现的。这些研究表明,总捕获强度的50%至85%是由于p波捕获( = 1)引起的。不幸的是,数据分析不允许提取明确的TME集,因此无法对理论结果进行严格的测试。在我的工作中,我们能够减少不确定性并扩大了偏振可观测值的测量角度范围。通过停止E 的氘核极化光束,我们获得了矢量和张量分析角A y 和T 20 的角度分布d (实验室)= 115 keV在重水冰目标中。数据分析除了s波(E2)捕获项外还包括 l = 1个分波,分别对应于电偶极子(E1)和磁四极子(M2)辐射。独特的拟合获得了s波(E2)捕获强度为总强度的55±8%,p波强度为29±6%(E1)和16±3%(M2)的结果。总计为45±7%。将测得的分析能力和TME分析的结果与改进的共振组模型计算进行了比较。尽管p波相位与实验确定的结果不一致,但是观察到的和计算出的跃迁幅度非常吻合,这将需要我们的分析与计算的进一步比较。最后,通过这项工作建立的p波强度导致了天体物理学S因子对于 2 H( d &ar; ,γ) 4 He反应比以前的最佳计算低2倍。

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