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Wat (wie) is cosmological$16963$ - definitie
HORIZON APPEARING ON A COSMOLOGICAL SCALE
Cosmological horizons; List of cosmological horizons; Hubble horizon; Cosmological Horizon
Cosmological constant
![Estimated ratios of [[dark matter]] and dark energy (which may be the cosmological constant<ref name="CC Definition"/>) in the universe. According to current theories of physics, dark energy now dominates as the largest source of energy of the universe, in contrast to earlier epochs when it was insignificant.](https://commons.wikimedia.org/wiki/Special:FilePath/080998 Universe Content 240 after Planck.jpg?width=200 "Estimated ratios of [[dark matter]] and dark energy (which may be the cosmological constant<ref name=\"CC Definition\"/>) in the universe. According to current theories of physics, dark energy now dominates as the largest source of energy of the universe, in contrast to earlier epochs when it was insignificant.")
CONSTANT REPRESENTING STRESS-ENERGY DENSITY OF THE VACUUM IN EINSTEIN'S EQUATION AND ACCOUNTS FOR THE RATE OF EXPANSION OF THE UNIVERSE
Cosmological Constant; Einstein's cosmological constant; Einstein's big blunder; Cosmic constant; Cosmological term; Cosmological constants
In cosmology, the cosmological constant (usually denoted by the Greek capital letter lambda: Λ), alternatively called Einstein's cosmological constant,
Cosmological horizon
A cosmological horizon is a measure of the distance from which one could possibly retrieve information. This observable constraint is due to various properties of general relativity, the expanding universe, and the physics of Big Bang cosmology.
Cosmic time
MEASURE OF TIME BY A PHYSICAL CLOCK WITH ZERO PECULIAR VELOCITY IN THE ABSENCE OF MATTER OVER-/UNDER-DENSITIES SINCE THE BIG BANG
Cosmological time; Draft:Cosmic time; User:Miladiouss/sandbox
Cosmic time, or cosmological time, is the time coordinate commonly used in the Big Bang models of physical cosmology.In mathematical terms, a cosmic time on spacetime M is a fibration t \colon M \to R.
Wikipedia
Cosmological horizon
A cosmological horizon is a measure of the distance from which one could possibly retrieve information. This observable constraint is due to various properties of general relativity, the expanding universe, and the physics of Big Bang cosmology. Cosmological horizons set the size and scale of the observable universe. This article explains a number of these horizons.
