Unfortunately, WIMPS are just a theory so far.
遗憾的是，这种wimp粒子目前只是理论假设。
Supporters of the idea believe a large number of WIMPS pass through the Earth every second.
这种理论的支持者相信每时每刻都有大量弱作用大质量粒子通过地球。
The new detectors are designed to be much better at distinguishing WIMPs from surface events.
设计这些新的探测器就是为了更好地区分弱作用大质量粒子与表面事件。
If Hooper's flavour of WIMPS exists then they should be efficiently captured by stars, including the Sun.
如果Hooper使用的WIMPs存在，那么它们会有效地被恒星，包括太阳所捕获。
Though scientists have no idea what it consists of, one popular theory is that dark matter is made up of WIMPs (Weakly Interacting Massive Particles).
虽然科学家还不清楚暗物质如何构成，不过一种通行的理论认为其由弱作用大质量粒子组成（WIMPs）
Discovering WIMPs is a big deal and you've got to be sure you're looking at the right thing.
探索弱作用大质量粒子是一件大事，必须明确自己没找错目标。
These annihilations are thought to occur when two WIMPs collide, generating gamma-rays which can be picked up by detectors such as those on board Fermi.
据称，在两个弱作用大质量粒子碰撞时会发生湮灭，并且放出伽马射线，类似费尔米卫星的探测器能够捕捉到这种信号。
When two WIMPs collide, they can annihilate each other, giving rise to other particles—such as positrons. The data from AMS so far match these predictions.
当两个大质量弱相互作用粒子碰撞时，它们会彼此消灭，从而产生另一些粒子——比如正电子。
A particle theory called "supersymmetry" predicts the existence of weakly interacting massive particles (WIMPs), which could be the particles of dark matter.
一种被称为“超对称性”的粒子理论预言了“弱作用重粒子”(WIMPs)的存在——它也许就是暗物质粒子。
Deep underground experiments on Earth have attempted to directly detect the weakly interacting particles (WIMPS) that scientists believe constitute dark matter.
科学家们相信是弱相互作用粒子(WIMPS)构成了暗物质，在地球上进行的深地下实验正试图直接探测到这种粒子。
Physicists have long wondered about dark matter. One of the most popular explanations is that it consists of weakly interacting massive particles, also known as WIMPs.
从很早以前开始，物理学界就一直在寻找关于暗物质的一切，一种最流行的探索途径是寻找WIMPs，即弱作用重粒子。
Their simulation starts about 50m years after the Big Bang, when the first galaxies formed, and calculates the interactions of a billion WIMPs over the intervening 13.7 billion years.
这个模型模拟的是自宇宙大爆炸后5千万年——第一个星系形成的时候，并且计算出了137亿年间数以10亿计WIMP的相互作用。
One possible explanation for these positrons is the mutual annihilation of the matter and antimatter forms of a type of dark matter called weakly interacting massive particles, also known as WIMPs.
对这些正电子有一个可能解释，就是它们来自同一种暗物质以正、反物质形式出现的一对粒子的碰撞（物质湮灭），这样的暗物质又被称为“大质量弱相互作用粒子”（WIMP）。
One possible explanation for these positrons is the mutual annihilation of the matter and antimatter forms of a type of dark matter called weakly interacting massive particles, also known as WIMPs.
对这些正电子有一个可能解释，就是它们来自同一种暗物质以正、反物质形式出现的一对粒子的碰撞（物质湮灭），这样的暗物质又被称为“大质量弱相互作用粒子”（WIMP）。
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