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Neutrino flavour states and the quantum theory of neutrino oscillations

机译:中微子风味态与中微子振荡的量子理论

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The definition and derivation of flavour neutrino states in the framework of standard quantum field theory is reviewed, clarifying some subtle points. It is shown that a flavour neutrino state that describes a neutrino produced or detected in a charged-current weak interaction process depends on the process under consideration and is appropriate for the description of neutrino oscillations as well as for the calculation of neutrino production or detection rates. Hence, we have a consistent framework for the description of neutrino oscillations and interactions in neutrino oscillation experiments. The standard flavour neutrino states are obtained as approximations which describe neutrinos in experiments that are not sensitive to the dependence of neutrino interactions on the neutrino mass differences. It is also shown that the oscillation probability can be derived either through the usual light-ray time = distance approximation or through an average of the spacetime-dependent oscillation probability over the unobserved propagation time.
机译:在标准量子场论的框架内,对风味中微子态的定义和推导进行了综述,阐明了一些微妙的地方。结果表明,描述在充电电流弱相互作用过程中产生或检测到的中微子的风味中微子状态取决于所考虑的过程,并且适合于描述中微子振荡以及计算中微子的产生或检测率。 。因此,我们有一个一致的框架来描述中微子振荡实验中的中微子振荡和相互作用。获得标准风味中微子状态,作为近似值,该状态描述了对中微子相互作用对中微子质量差异的依赖性不敏感的实验中的中微子。还表明,可以通过通常的光线时间=距离近似或通过在未观察到的传播时间上依赖于时空的振荡概率的平均值来得出振荡概率。

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