The order of magnitude of time and space in the universe

(astronomy) That part of any redshift that is accounted for by the expansion of spacetime following the Big Bang

(astronomy) The distance from an observer in a universe beyond which it is impossible for the observer to see, as the light (or other luminal particles) cannot have travelled that distance over the current age of that universe.

(physics) A term added by Albert Einstein to his equations of general relativity in order to account for a supposed static universe, since used to describe vacuum energy as a form of dark energy.

(theology, philosophy) A type of argument for the existence of God arguing that since every thing and event that begins at a point in time has a cause, there must be an uncaused first cause.

plural of cosmological argument

plural of cosmological city

plural of cosmological horizon

plural of cosmological decade

plural of cosmological constant