Realistic arrival time distribution from an isotropic light source

Realistic arrival time distribution from an isotropic light source
复制标题

各向同性光源的真实到达时间分布

DOI:
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发表时间:
2005
期刊:
arXiv: Astrophysics
影响因子:
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通讯作者:
M. Ribordy
M. Ribordy
中科院分区:
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文献类型:
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作者:
G. Japaridze;M. Ribordy

文献摘要

被引文献

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高能中微子望远镜中的事件重建是基于探测到的光子通过均匀的散射介质传播到距离其发射点一定距离的时延分布的表达式。 考虑具有有限时间分辨率的实际探测器,我们推导出被探测光子时延的概率密度函数的表达式。计算并讨论了该函数的渐近性质及其相应的累积概率分布。
The event reconstruction in high energy neutrino telescopes is based on the expression of the time delay distribution of the detected photons propagating to some distance from their emission point through a uniform and scattering medium. Considering a realistic detector with a finite time resolution, we derive an expression for the probability density function of the time delay of detected photons. The asymptotic properties of this function as well as its corresponding cumulative probability distribution are calculated and discussed.