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Shedding Light on Dark Matter

机译:在暗物质上发光

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The "stuff" that makes up the universe is mostly invisible. Matter that we can see or detect, such as the substances that make up the planets, stars, and interstellar dust, comprises only 4 percent of the total. The rest of the mass in the universe, most scientists believe, consists of dark matter—matter of unknown composition that does not emit or reflect electromagnetic radiation and is therefore difficult to observe directly. Determining the nature of this "missing mass" is one of the most important problems in modern cosmology and particle physics. Several kinds of particles have been proposed as dark-matter candidates, and many experiments and searches are under way to detect them. One candidate is some kind of a weakly interacting massive particle (WIMP). Because WIMPs do not interact with electromagnetism or interact strongly with matter, they are nearly impossible to detect directly.
机译:组成宇宙的“东西”大部分是不可见的。我们可以看到或检测到的物质,例如构成行星,恒星和星际尘埃的物质,仅占总数的4%。大多数科学家认为,宇宙中的其余质量都是由暗物质组成的,暗物质是未知成分,不会发射或反射电磁辐射,因此很难直接观察到。确定这种“缺失质量”的性质是现代宇宙学和粒子物理学中最重要的问题之一。已经提出了几种颗粒作为暗物质候选物,并且正在进行许多实验和搜索以检测它们。一个候选对象是某种弱相互作用的大颗粒(WIMP)。由于WIMP不与电磁相互作用或与物质强烈相互作用,因此几乎不可能直接检测到它们。

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