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Indirect studies of astrophysical reaction rates through transfer reactions

机译:通过转移反应间接研究天体物理反应速率

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摘要

The work in this thesis describes two experiments which use transfer reactions to perform spectroscopic studies of nuclei in order to improve reaction rates in astrophysical environments.udThe first experiment is an indirect study of the 34S(p,γ)35Cl reaction rate at energies relevant to classical novae temperatures. By reducing uncertainties in this reaction it may be possible to use 32S/34S isotopic ratio as a diagnostic tool to determine pre-solar grain paternity. A study of the 34S(3He,d)35Cl transfer reaction was performed to identify energy levels in the astrophysically relevant energy region and assign spin and parity to these new states. A new reaction rate has been calculated from this spectroscopic information and is the first experimental measurement of the 34S(p,γ)35Cl reaction rate. Using this new rate it was concluded that it is now possible to determine the paternity of pre-solar grains using the 32S/34S isotopicudratio.udThe second experiment measured two proton transfer reactions, (3He,d) and (α,t), with the aim of making spin assignments of states above the neutron threshold in 27Al. Combined with information from complementary experiments this information would be used to calculate new 26Al(n,p/α) reaction rates. Direct comparison ofudthe two transfer reactions should allow for low and high spin states to be identified, however due to lower than expected cross sections useful information could not beudextracted from the (α,t) reaction. The experimental resolution was insufficient to resolve individual states with the (3He,d) reaction, however due to the selectivityudof the reaction it appears that many of the previously known states show low spin behaviour and are likely not relevant to the reaction rate at astrophysicaludtemperatures. In addition, the non-observation of 23 states known to exist in 27Al may indicate they are high spin and further measurements of these states should beudperformed in order to calculate new 26Al(n,p/α) reaction rates.
机译:本文的工作描述了两个使用转移反应对原子核进行光谱研究以提高在天体环境中的反应速率的实验。 ud第一个实验是在能量相关的情况下间接研究34S(p,γ)35Cl反应速率到新星的温度。通过减少该反应的不确定性,有可能使用32S / 34S同位素比作为诊断工具来确定太阳前谷物的亲子关系。进行了34S(3He,d)35Cl转移反应的研究,以确定与天体相关的能量区域中的能级,并将自旋和奇偶性赋予这些新状态。从该光谱信息计算出新的反应速率,这是对34S(p,γ)35Cl反应速率的首次实验测量。使用这一新速率得出的结论是,现在可以使用32S / 34S同位素比值确定太阳前晶粒的亲子关系。 ud第二个实验测量了两个质子转移反应(3He,d)和(α,t ),以使自旋分配状态高于27Al中子阈值。结合来自补充实验的信息,该信息将用于计算新的26Al(n,p /α)反应速率。两个转移反应的直接比较应该可以识别出低和高自旋态,但是由于横截面低于预期,因此无法从(α,t)反应中提取有用的信息。实验分辨率不足以解决(3He,d)反应的单个状态,但是由于该反应的选择性 ud,看来许多先前已知的状态均显示出低自旋行为,并且可能与反应速率无关。天体高温。此外,未观察到27Al中存在的23种状态可能表明它们具有高自旋性,应对这些状态进行进一步的测量以计算新的26Al(n,p /α)反应速率。

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    Gillespie Stephen;

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