The whole universe was a super-hot soup of radiation filled with these particles.
整个宇宙就像一碗充满这些粒子的超热辐射汤。
The whole universe was a super hot soup of radiation filled with these particles.
整个宇宙是充满这些粒子的热辐射汤。
We call these particles atoms.
我们把这些粒子叫做原子。
They count where these particles hit the screen.
当粒子撞击到屏幕的时候就记录一次。
Heat sets these particles in random motion.
热量使这些粒子作随机运动。
To be sure, you can't see these particles.
可以肯定，你不能看到这些微粒。
Both of these particles can produce ion pairs.
这两种粒子都能产生离子对。
When these particles hit the moon, most stick to the lunar surface.
当这些粒子撞到月球时，多数粘在月球表面上。
Until now, scientists were unsure of the net effect of these particles.
在这之前，科学家还不能确定这些颗粒造成的净效应。
Some of these particles may not have been witnessed by scientists before.
其中的一些粒子在之前也许一直没有被科学家们观测到。
Cherenkov light comes from these particles when the speed of light is exceeded.
切伦科夫光来自光速被超过时的这些粒子。
We are protected from these particles by the Earth's magneticfield and atmosphere.
我们被地球磁场和大气层保护免受这些粒子流的伤害。
All these particles were subsequently found, with precisely the predicted properties.
这些粒子后来都找到了，性质也与预测完全相符。
As the universe expanded and cooled, some of these particles merged to form neutrons and protons.
在宇宙的扩大与冷却的过程中，这些粒子的一部分渐渐融合并组成了中子与质子。
If these particles really can combust spontaneously, LBNF stands a fair chance of spotting it.
如果这些颗粒真的能自燃，那么LBNF极有可能可以观察到这种变化。
Once the larger of these particles get big enough to have a nontrivial gravity, their growth accelerates.
一旦这些较大的颗粒大到具有了非平凡重力，他们的增长便会加速。
Meanwhile, several other experiments are joining international efforts to hunt for signals from these particles.
同时，许多其他的实验也加入了捕捉(暗物质)粒子信号的国际努力中。
All of these particles and gases contribute to global warming and some are dangerous air pollutants that can lead to respiratory disease.
所有这些微粒与气体不但造成了全球变暖，其中有一些还是危险得能引发呼吸系统疾病的空气污染物。
In addition, these particles were so small they could have melted quickly inside jet engines, potentially causing them to fail mid-flight.
此外，这些颗粒非常细小，有可能很快熔化进入喷气引擎，造成空中停车。
Some of these particles are stable and form the normal matter, the others live for fractions of a second and then decay to the stable ones.
这些粒子中的一部分是稳定的并且构成了普通物质，其它的只存在一秒钟的几分之一，然后衰变为稳定粒子。
Scientists at the Cern lab in Geneva fired a beam of these particles through 450 miles of rock towards detectors in the Gran Sasso lab in Italy.
位于日内瓦的欧洲粒子物理研究所的科学家们向450公里外意大利格兰萨索地下实验室的探测器发射了一束中微子。
When they are applied to a surface, these particles block the minute crevices in it, reducing the scope for dirt, moisture and bacteria to cling to the surface.
当这些颗粒覆盖到某一表面时，就能堵塞表面细缝，从而减少灰尘、水分和细菌的黏附。
Both the emulsion stability experiments and the drop coalescence experiments are performed to evaluate the contribution of these particles to emulsification.
为评价这些微粒对乳化稳定性的贡献，分别开展了乳状液稳定性实验和液滴聚并实验。
However, try as hard as they might, scientists have yet to detect any of these particles, even with tests designed specifically to target their predicted properties.
可是，不管科学家如何努力，甚至用专门设计出的，检测其预期性质的实验，也没能探测出任何此类粒子。
Writing in the journal Diabetes Care (PDF), a team of researchers looked at the most insidious of these particles -- only those smaller than 2.5 micrometers in diameter.
在杂志《糖尿病治疗》中（PDF），一组研究人员研究了最容易被忽视的一些微粒——仅限于直径小于2.5微米的。
The LHC has a good chance of making these particles, but if they are six times as common as ordinary matter in outer space then it ought to be possible to detect them in the wild, as it were.
LHC很有可能会制造出这些微粒，但既然太空中的暗物质是普通物质的六倍之多，那么在自然界中，我们也应该可以观测到它们。
Hooper and Linden believe that these particles interact with the galaxy's magnetic field to produce a haze of radiation - and have modelled what they expect this radiation profile to look like.
Hooper和Linden认为，就是这些粒子与银河系磁场的相互作用产生了辐射薄雾。他们已经建立了他们预计的辐射轮廓的模型。
These particles do not resile but they unite after they collide.
这些粒子没有弹力，但碰撞以后它们会结合到一起。
These particles do not resile but they unite after they collide.
这些粒子没有弹力，但碰撞以后它们会结合到一起。
应用推荐