Hussain S, Marfatia D, McKay D W, Seckel D
Department of Physics and Astronomy, University of Delaware, Newark, DE 19716, USA.
Phys Rev Lett. 2006 Oct 20;97(16):161101. doi: 10.1103/PhysRevLett.97.161101. Epub 2006 Oct 17.
We examine the dependence of event rates at neutrino telescopes on the neutrino-nucleon cross section for neutrinos with energy above 1 PeV, and contrast the results with those for cosmic ray experiments. Scaling of the standard model cross sections leaves the rate of upward events essentially unchanged. Details, such as detector depth and cross section inelasticity, can influence rates. Numerical estimates of upward shower, muon, and tau event rates in the IceCube detector confirm these results.
我们研究了能量高于1 PeV的中微子在中微子望远镜中的事例率对中微子-核子截面的依赖性,并将结果与宇宙射线实验的结果进行对比。标准模型截面的标度变换使向上事例的发生率基本保持不变。诸如探测器深度和截面非弹性等细节会影响发生率。对冰立方探测器中向上簇射、μ子和τ子事例率的数值估计证实了这些结果。