baryonic
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例句
Non- baryonic matter , as implied by the name, is any sort of matter that is not primarily composed of baryons.
而非重子物质则是从质量上来看主要不是由重子组成的物质，比如中微子、自由电子、光子等等。
Most of the normal (baryonic) mass is in the hot gas detected by the Chandra X-Ray Observatory, shown in pink.
大部分正常（重子）的物质是列于粉红色，热气体检测射线的钱德拉天文台的X。
Small as the percentage might be, half of the ordinary baryonic matter is unaccounted for.
这可能是个很小的百分比，有一半的普通重子物质还没有考虑到。
Whereas each CDM particle conserves its energy from then on, the baryonic gas is able to emit radiation.
虽然每一个CDM粒子的能量从此不会改变，重子气体却仍能辐射电磁波。
A byproduct of this part is the distribution of the (baryonic) mass-to-light ratio of elliptical galaxies.
这部分的一个副产品是椭圆星系的（重子）质光比分布。
Scientists call ordinary matter "baryonic matter" because protons and neutrons are subatomic particles called baryons.
科学家把这些常见物统称为“重物质”，因为质子和中子都属于亚原子结构的重子。
Over the years, we've pretty much ruled out all sorts of baryonic dark matter possibilities like brown dwarfs or black holes.
多年来，我们常常将存在各种重子暗物质（如：褐矮星或黑洞）的可能性排除在外。
Scientists call them baryonic matters, as protons and neutrons are called baryons in sub-atomic particles.
科学家们把它们称为“重子物质”，因为质子和中子在亚原子粒子中被称为“重子”。
Dark matter: this generally refers to "exotic" non-baryonic matter that interacts only weakly with ordinary matter.
暗物质：这一般是指“外来的”非重子物质，与普通物质只有较弱的的相互作用。
A significant amount of non- baryonic , cold matter is necessary to explain the large-scale structure of the universe.
一重要量的非重子、冷物质是必须的、用来解释大范围的宇宙结构。
Astronomers split non-baryonic dark matter into two categories: hot and cold.
天文学家把非重子暗物质分成两类：热质和冷质。
however, it may also include exotic species of non- baryonic dark matter, such as supersymmetric particles, axions or black holes.
重的可能组成非重子暗物质的物质可能有超对称粒子、黑洞等。
Baryonic matter: In this cosmological context, this is "ordinary matter" composed primarily of protons, neutrons and electrons.
重子：这是“传统物质”，主要由质子，中子和电子组成。
Possibilities involving normal baryonic matter include brown dwarfs or perhaps small, dense chunks of heavy elements;
涉及常态重子物质包括褐矮星或者也许小的、密集块的重元素的可能性；
Merging of galaxy haloes must preserve the proportionality between black hole mass and baryonic mass;
星系晕的合并必须保持与黑洞的质量和重子物质的比例；
Non-Baryonic - hot dark matter (HDM) and cold dark matter (CDM)
非重子-热的暗物质（HDM）及冷的暗物质（CDM）
