baryonic

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

Most of the normal (baryonic) mass is in the hot gas detected by the Chandra X-Ray Observatory, shown in pink.

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

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

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

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

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

Scientists call them baryonic matters, as protons and neutrons are called baryons in sub-atomic particles.

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

A significant amount of non- baryonic , cold matter is necessary to explain the large-scale structure of the universe.

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

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

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

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

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

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