网络冰立方中微子天文台 网络释义 1. 冰立方中微子天文台 ...在南极冰川8000英里深处完工,该天文台被称为南极冰立方中微子天文台(IceCube Neutrino),用于探测难以捉摸的次原子 … it.sohu.com|基于2个网页
During the public Kaggle competition “IceCube – Neutrinos in Deep Ice”, thousands of reconstruction algorithms were created and submitted, aiming to estimate the direction of neutrino events recorded by the IceCube detector. Here we describe in detail the three ultimate best, award-winning solutions...
We investigate the IceCube detection potential of very high energy neutrinos from blazars, for different classes of "hadronic" models, taking into account the limits imposed on the neutrino flux by the recent Fermi telescope observations. Assuming the observed gamma-ray emission is produced by the ...
(PhysOrg.com) -- On Saturday, December 18, the IceCube Neutrino Observatory sank the last of 86 strings of sensitive photodetectors to a depth of almost two and a half kilometers in the ice at the South Pole, marking completion of the huge neutrino teles
IceCube is a large neutrino telescope of the next generation to be constructed in the Antarctic Ice Sheet near theSouth Pole. We present the conceptual design and the sensitivity of the IceCube detector to predicted fluxes of neutrinos, both atmospheric and extra-terrestrial. A complete simulation ...
(PhysOrg.com) -- On Saturday, December 18, the IceCube Neutrino Observatory sank the last of 86 strings of sensitive photodetectors to a depth of almost two and a half kilometers in the ice at the South Pole, marking completion of the huge neutrino teles
Posted in Featured, Interest, Science, SliderTagged ANITA, black holes, IceCube Neutrino Observatory, neutrinos Search Search for: Never miss a hack Follow on facebook Follow on twitter Follow on youtube Follow on rss Contact us Subscribe If you missed it The “Unbreakable” Beer Glasses Of...
IceCube公布首度搜索太阳大气微中子的结果是：还没找到 位在南极大陆的冰块微中子天文台（或译冰立方微中子天文台，IceCube）是第一个搜索太阳大气微中子（atmospheric neutrino）的观测站，这对了解太阳磁场及宇宙线（cosmic ray）如何在内太阳系穿梭有很重要的作用，甚至可以提供有关太阳暗物质研究的消息。经过7年奋斗...
We have determined the currently allowed regions of the parameter spaces of two representative models of diffuse neutrino flux from active galactic nuclei (AGN): one by Koers & Tinyakov (KT) and another by Becker & Biermann (BB). Our observable has been the number of upgoing muon-neutrinos...