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Sensitivity Studies Using Globes

机译:使用地球仪进行敏感性研究

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Neutrino oscillation occurs if neutrinos have masses and if they mix among each other. t his phenomenon would be in close analogy to the experimentally observed mixing in quark sector. Neutrino oscillations are therefore very interesting in the context of elementary particle physics. Neutrino oscillation in matter is probably the reason for the observed deficit of solar neutrino flux . t he search for neutrino oscillation is the only way to investigate even for very small difference of neutrino masses. t he evidence of small but non vanishing neutrino masses represent one of the few clear indications of the physics beyond standard model. t he findings of nonzero neutrino masses by Super- k amiokande in 1998 triggered a huge interest of experimentalists in neutrino physics. In the present article after discussing the theoretical background concerning massive neutrinos and their status in standard model, latest important long baseline experiments dealing with neutrino oscillations have been discussed. It has been tried to show the important link between the physics behind neutrino oscillation and the software used ( g loBES).
机译:如果中微子具有质量并且彼此混合,就会发生中微子振荡。他的现象与夸克区的混合实验非常相似。因此,中微子振荡在基本粒子物理学的背景下非常有趣。物质中微子的振荡可能是太阳中微子通量不足的原因。寻找中微子振荡是研究中微子质量差异很小的唯一方法。中微子质量小的但没有消失的证据代表了超出标准模型的物理学的少数几个明确指标之一。 Superk amiokande在1998年发现的非零中微子质量引起了中微子物理学界的极大兴趣。在讨论了有关中微子的大量理论背景及其在标准模型中的地位后,本文讨论了最新的重要中长期基线实验。已尝试显示中微子振荡背后的物理原理与所用软件(g loBES)之间的重要联系。

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