The result is almost a fluid of baryonic matter and radiation.

结果是产生一种带辐的重子物质流体。

What we observe is the baryons, the regular stuff.

我们观测到的是重子即常规物质。

And as the two giants struggle, they heave this fluid back and forth — creating massive waves called baryonic acoustic oscillations.

当这两个巨人搏斗时，它们揉捏着这流体——产生名为重子声振荡的巨大波纹。

We expect the universe to be made up of 5 percent baryonic matter.

我们预计宇宙由 5% 的重子物质组成。

It doesn't interact with or omit electromagnet radiation and we know that it can't be matter as if it was it would contain particles called baryons which we'd be able to detect it through reflected light.

它不与电磁辐作用，也不忽略电磁辐，我们知道它并不重要，因为它包含称为重子的粒子，我们可以通过反光检测到它。

The dark galaxy discovered by FAST has a baryonic  mass of 100 million solar masses and a dynamic mass of 5.1 billion solar masses.

FAST发现的暗星系拥有1亿太阳质量的重子物质和51亿太阳质量的动力质量。

And this is the first time scientists have confidently observed a baryon containing two heavier flavors of quark.

这是科家首次有信心地观测到含有两种较重夸克的重子。

To do so, Chae studied the statistical relation between the observed  centripetal acceleration of particles in motion and the expected Newtonian acceleration from the  distribution of baryonic matter in the galaxies.

为此，车研究了运动中粒子观测到的向心加速度与来自星系中重子物质分布预期的牛顿加速度之间的统计关系。

Inside a baryon like a proton, the three light quarks are pretty evenly balanced and zip around each other.

在一个像质子这样的重子内部，三个轻夸克当均衡，并且绕着对方快速移动。

Adding all of that neutral hydrogen gas into our baryon budget brings us almost to 50 percent.

将所有这些中性氢气加到我们的重子预算中，使我们几乎达到 50%。

Now just imagine we could do something very similar to find all the ionized baryons in the universe.

现在想象一下，我们可以做一些非常似的事情来找到宇宙中所有的电离重子。

We can't see it, but its existence can be inferred because of its effect on surrounding baryonic matter.

我们虽然看不见它，但可以通过它对周围重子物质的效应推断其存在。

No, that's only like 10 or 20 percent of all the baryonic matter.

不， 那只是所有重子物质的 10% 或 20%。

It's a graph between the baryonic mass of the galaxy to its rotation velocity.

这是一张星系的重子质量与其旋转速度之间关系的图表。

The Standard Model predicts the existence of these baryons, so they weren’t, like, a huge surprise.

标准模型预测了这些重子的存在，所以它们并不是什么大惊喜。

We’ve observed some heavier baryons before.

我们之前观察到过一些更重的重子。

Furthermore, as per different theories,   the majority of dark matter is thought to be non-baryonic.

此外，根据不同的理论，大部分暗物质被认为是非重子性的。