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Galaxies form when the density of matter exceeds some critical value.
What is normally sought after is the density of matter in the universe (which is the mass per unit volume).
open universe Geometry that the universe would have if the density of matter were less than the critical value.
If we imagine the universe shrinking backward, like a film in reverse, the density of matter and energy rises toward infinity as we approach the moment of origin.
It states that the strength of a celestial object's gravitational field is determined by the density of matter it contains: the higher the density, the stronger the gravity.
Its departure from Euclidean space is measured by a "curvature" that depends on the density of matter.
Depending on the density of matter in the universe, this puts the date of the Big Bang between 8 billion and 12 billion years ago.
closed universe Geometry that the universe as a whole would have if the density of matter is above the critical value.
radiation-dominated universe Early epoch in the universe, when the density of radiation in the cosmos exceeded the density of matter.
singularity A point in the universe where the density of matter and the gravitational field are infinite, as in the center of a black hole.
The density of matter in these wrinkles was slightly greater compared to surrounding areas and this difference was magnified during inflation, allowing them to attract even more matter.
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Since I tried Ludwig back in 2017, I have been constantly using it in both editing and translation. Ever since, I suggest it to my translators at ProSciEditing.

Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com