电子中微子

比如，一个地方的核反应堆中释放的电子中微子，可以以μ中微子的形式出现在另一个地方的探测器中。

An electron neutrino , say , can emerge from a nuclear reactor in one place and appear in a detector somewhere else as a muon neutrino .

利用超新星爆发测量电子中微子静止质量

Measurement of electron neutrino mass by supernova neutrino bursts

自从被提出以来，直到26年后的1956年，才由Reines和Cowan首次探测到了来自反应堆的反电子中微子。

The first detection of electron anti-neutrinos from reactor was made by Reines and Cowan in the year 1956 , almost 26 years after neutrino was postulated .

在模拟过程中，以台北国圣核电厂的反应堆为基础，建立了简化的反应堆模型，通过模拟计算求出了电子中微子的通量。

A simplified model was constructed according to the reactor at the Kuo-Sheng power plant in Taipei .

为充分利用反应堆开展对电子中微子各项物理属性的研究，首次对反应堆电子中微子通量进行了模拟计算。

For further research work on reactor neutrino experiment , we performed the first simulation of the emissions of electron neutrinos from a nuclear reactor .

物理学家们知道，中微子至少有三种，由于其不同的亚原子起源，中微子被分为电子中微子、μ中微子和τ中微子。

Physicists know that neutrinos come in at least three flavors , known as electron , muon and tau neutrinos , depending on their subatomic origin .

中微子振荡机制已经被证实为太阳中微子缺失问题的合理解释，作为理论基础，我们在第三章中重点介绍了中微子振荡理论，并给出电子中微子在太阳内部具体传播行为的表述。

The neutrino oscillation mechanism has been confirmed as the solution to the solar neutrino problem . We give a detailed introduction of the theory of neutrino oscillations and also a detailed description of solar neutrinos propagation in solar interior .

τ轻子的发现和电子反中微子的首次观察&1995年诺贝尔物理奖介绍

Discovery of the τ Lepton and Electron Antineutrino Awarded the 1995 Nobel Physics Prize

余下的一个描述电子-中微子和τ介子-中微子之间振荡的θ13被证明是难以捉摸的。

The remaining one , theta-13 , which governs the relationship between electron - and tau-neutrinos , has proved elusive .

本文提出一种从氚衰变β谱确定电子反中微子静止质量的新型结构β谱仪。

A method is described for measuring the beta spectrum from tritium decay in order to determine the electron - antineutrino rest mass .

束缚电子对~7Be太阳中微子流量的影响

Effect of bound electron capture on ~ 7Be solar neutrino flux

束缚电子屏蔽效应对中微子俘获反应的影响

Effect of Bound Electron Screening on Neutrino Capture

另一种可能产生的背景电子是对探测中微子暗物质的潜在威胁，它是通过太阳中微子与靶材料中的电子散射所产生的电子。

Another possible background , which is a potential threat to the detection of vs dark matter , is the electron event produced by the scattering of solar neutrinos with electrons in target matter .