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Cosmologists puzzle over mystery in the cosmos

机译:宇宙学家对宇宙中的奥秘感到困惑

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It may not be the ethereal spirit that it looks like, but to cosmologists it is still rather surprising: two "hot spots" (yellow/red) of cosmic rays. The hot spots were observed using the Milagro telescope in the Jemez mountains near Los Alamos in the US – the first observatory capable of continuously monitoring the northern sky for cosmic rays. As cosmic rays bombard nuclei in the atmosphere they produce showers of secondary particles. Milagro detects these particles as they fall into a huge pool of water and create flashes of Cerenkov radiation, which can be picked up by photomultipliers. The cosmic-ray hot spots above are unusual because of their relatively low energy: at about 10 TeV one would expect galactic magnetic fields to still be able to scramble the paths of cosmic rays, so that they would appear with a random distribution across the sky. Physicists in the Milagro team are unsure where the hot spots come from, but suggest that they could be the result of a special magnetic-field structure that guides the cosmic rays to Earth. Another possibility is that the cosmic rays are neutral particles such as neutrons, although these have lifetimes too short to make this likely (Phys. Rev. Lett. 101 221101). "We are nearing the centenary of the discovery of cosmic rays and we still do not have proof of where they come from," says Milagro teammember John Pretz. "If these hot spots are due to a source of cosmic rays, then it would be the solution to a 100-year-old riddle. It is also exciting because, for the first time, we are starting to see isolated features in the cosmic-ray sky, and that can help us understand their origin."
机译:它可能看起来并不像是空灵,但对于宇宙学家来说,这仍然令人惊讶:两个宇宙射线的“热点”(黄色/红色)。使用米拉格罗(Milagro)望远镜在美国洛斯阿拉莫斯附近的杰米兹山脉观测到了热点,这是第一家能够连续监测北部天空宇宙射线的天文台。当宇宙射线轰击大气中的原子核时,它们会产生次级粒子的阵雨。当这些微粒落入巨大的水池中并产生切伦科夫辐射的闪光时,Milagro会检测到这些微粒,这些微粒可以被光电倍增管拾取。上面的宇宙射线热点由于能量相对较低而很不寻常:在大约10 TeV处,人们会期望银河磁场仍然能够扰乱宇宙射线的路径,因此它们会以随机分布的方式出现在天空中。 Milagro小组的物理学家不确定热点的来源,但建议它们可能是将宇宙射线引导到地球的特殊磁场结构的结果。另一种可能性是宇宙射线是中子等中性粒子,尽管它们的寿命太短而无法实现(Phys。Rev. Lett。101 221101)。 Milagro团队成员约翰·普雷兹(John Pretz)说:“我们已经接近发现宇宙射线的百年历史,我们仍然没有关于它们来自何处的证据。” “如果这些热点是由于宇宙射线源引起的,那么这将是解决一个已有100年历史的谜语的方法。这也是令人兴奋的,因为,这是我们第一次开始看到宇宙中孤立的特征。射线的天空,这可以帮助我们了解它们的起源。”

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