c, speed of lightThe speed that light travels in a vacuum. It is about 3 x 108 m/s (186,000 miles/s).
Closed UniverseA universe where the geometry of space closes upon itself like the surface of a sphere.
clusterClusters are fixed length blocks of bytes that store data for Microsoft operating systems.
Constant of ProportionalityWhen scientists or theoreticians find a mathematical relationship between two quantities, they design an equation, so that, for example, if one quantity…
Cosmic Microwave Backgroun (CMB)Radiation filling the universe, remaining from the early, hot phase. (It is sometimes called the "primal glow.") Today this radiation has cooled to 2.
Cosmological Constant, ΛThe energy density of the smooth vacuum. Eisntein introduced it as a component of the universe but later withdrew it.
Cosmological PrincipleA principle invoked in cosmology that severely restricts the large variety of possible cosmological theories: On large scales, the Universe is homogeneous…
CosmologyThe study of the universe as a whole, of the contents, structure, and evolution of the universe from the beginning of time to the future.
Coupled to RadiationMatter, such as charged particles, that is strongly affected by radiation.
Critical DensityThe density of matter/energy that would just halt the expansion of the universe. The dividing line between a collapsing and an ever-expandinguniverse.
Curvature of SpacetimeAccording to Einstein's General Theory of Relativity, mass curves space and time.