neutrinos

美 [nuˈtrinoʊz]英 [nju(ː)ˈtriːnəʊz]
  • n.中微子
  • neutrino的复数
neutrinosneutrinos
  1. Neutrinos are subatomic particles , and while there are plenty in the Universe , they 're very hard to detect .

    中微子是次原子粒子,虽然宇宙中有大量中微子,但它们很难被探测到。

  2. This massive space telescope is what it takes to detect the Universe 's best kept secrets – neutrinos – also nicknamed ‘ ghost particles ' .

    科学家们需要用这台大型太空望远镜来探测宇宙中最隐蔽的秘密,即中微子,别名“幽灵粒子”。

  3. Scientists are hoping that by capturing the elusive8 neutrinos , they 'll be able to better understand the Universe – finding out how it came to be and how it 's evolved to what we know today .

    科学家们希望,通过捕捉这些难以找到的中微子,他们能够更好地了解宇宙,并探索宇宙的诞生及演变至今的过程。

  4. Therefore , the study of neutrino is of great significance .

    因此,研究探索中微子意义重大。

  5. One New Experimental Method of Detection Neutrino Static Mass

    中微子静止质量测量新方法及讨论

  6. The Structure of a Neutrino and Its Structure Function

    中微子结构及其结构函数

  7. Development of a New Detector for Solar Neutrino Detection

    新型太阳中微子闪烁探测器的研制

  8. Current Progress on Study of Solar Neutrino Problem

    太阳中微子问题研究进展

  9. Neutrino Compounding and Oscillation Parameters Calculation and Physical Mechanism Analysis

    中微子混合、振荡参数计算及物理机制分析

  10. Study of the mechanism of neutrino communication

    中微子通讯机理探讨

  11. This paper summarizes the history and applications of neutrinos .

    概述了中微子的历史以及应用。

  12. The study of mass 、 mixed and oscillation of neutrino

    中微子的质量、混合和振荡研究

  13. The history and status of neutrino mass measurements are summarized in this paper .

    本文介绍中微子质量测量的历史和现状。

  14. The Physical Sources for Neutrino to Obtain Mass and Charge

    中微子获得质量和电荷的物理根源

  15. Effect of spin on the black hole entropy due to neutrinos

    中微子的自旋对黑洞熵的影响

  16. A New Contribution to the Solar Neutrino Problem

    对太阳中微子丢失之谜研究的一个新贡献

  17. And that would mean plenty of work for neutrino physicists .

    这就意味着中微子的物理学家将需要做大量的工作。

  18. The researchers said they observed about fifteen thousand neutrino events .

    据研究员说,他们在目的地观察到了一万五千个微中子。

  19. The neutrino , although not directly observed , was a theoretical necessity .

    当时中微子虽然还没有直接观察到,但它的存在有理论上的必然性。

  20. Statistically , your first neutrino interactionprobably happens somewhere around age ten .

    从统计学角度来看,中微子第一次撞击到我身体里的某个原子应该是在我10岁左右的时候。

  21. One new method of measuring neutrino helicity

    一个测量中微子螺旋性的新方法

  22. The rest mass of neutrinos and clustering in the early universe

    有静质量中微子对宇宙早期成团过程的影响

  23. A study on neutrino theory

    中微子理论的新探讨

  24. The formation and the structure of the neutrino astronomical objects

    中微子天体的形成及其结构

  25. Precise Measurement of Solar Neutrino Oscillation Parameters and Analysis of Sub-leading Effects

    太阳中微子振荡参数的精确测量和次级效应分析

  26. We then introduce the high energy neutrino emission from GRBs .

    然后,我们介绍了伽玛暴的高能中微子辐射。

  27. At the same time , different methods are used to measure and calculate the mass of the neutrino .

    于是一些理论也试图赋予中微子以质量,同时人们也在用不同的方法来测量和计算中微子的质量。

  28. The thought process of the discovery of Neutrino

    中微子发现的思维过程

  29. How the Neutrino in Collapse Phase Affect Type ⅱ Supernova Explosion

    坍缩阶段中微子对II型超新星爆发的影响

  30. Discussion and analysis of goldhaber 's neutrino helicity experiment measuring results

    关于M.Goldhaber中微子螺旋性测量结果的分析和讨论