baryonic

baryonic

美 　英

• 網絡重子的

例句

Non- baryonic matter , as implied by the name, is any sort of matter that is not primarily composed of baryons.

而非重子物質則是從質量上來看主要不是由重子組成的物質，比如中微子、自由電子、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）的物質是列于粉紅色，熱氣體檢測射線的錢德拉天文臺的X。

Small as the percentage might be, half of the ordinary baryonic matter is unaccounted for.

這可能是個很小的百分比，有一半的普通重子物質還沒有考慮到。

Whereas each CDM particle conserves its energy from then on, the baryonic gas is able to emit radiation.

雖然每一個CDM粒子的能量從此不會改變，重子氣體卻仍能輻射電磁波。

A byproduct of this part is the distribution of the (baryonic) mass-to-light ratio of elliptical galaxies.

這部分的一個副產品是橢圓星系的（重子）質光比分布。

Scientists call ordinary matter "baryonic matter" because protons and neutrons are subatomic particles called baryons.

科學家把這些常見物統稱為“重物質”，因為質子和中子都屬于亞原子結構的重子。

Over the years, we've pretty much ruled out all sorts of baryonic dark matter possibilities like brown dwarfs or black holes.

多年來，我們常常將存在各種重子暗物質（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.

科學家們把它們稱為“重子物質”，因為質子和中子在亞原子粒子中被稱為“重子”。

Dark matter: this generally refers to "exotic" non-baryonic matter that interacts only weakly with ordinary matter.

暗物質：這一般是指“外來的”非重子物質，與普通物質只有較弱的的相互作用。

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、冷物質是必須的、用來解釋大范圍的宇宙結構。

Astronomers split non-baryonic dark matter into two categories: hot and cold.

天文學家把非重子暗物質分成兩類：熱質和冷質。

however, it may also include exotic species of non- baryonic dark matter, such as supersymmetric particles, axions or black holes.

重的可能組成非重子暗物質的物質可能有超對稱粒子、黑洞等。

Baryonic matter: In this cosmological context, this is "ordinary matter" composed primarily of protons, neutrons and electrons.

重子：這是“傳統物質”，主要由質子，中子和電子組成。

Possibilities involving normal baryonic matter include brown dwarfs or perhaps small, dense chunks of heavy elements;

涉及常態重子物質包括褐矮星或者也許小的、密集塊的重元素的可能性；

Merging of galaxy haloes must preserve the proportionality between black hole mass and baryonic mass;

星系暈的合并必須保持與黑洞的質量和重子物質的比例；

Non-Baryonic - hot dark matter (HDM) and cold dark matter (CDM)

非重子-熱的暗物質（HDM）及冷的暗物質（CDM）