51Թ

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cosmological constant

noun

Astronomy.
  1. a term introduced by Einstein into his field equations of general relativity to permit a stationary, nonexpanding universe: it has since been abandoned in most models of the universe.


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51Թ History and Origins

Origin of cosmological constant1

First recorded in 1925–30
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Example Sentences

Examples have not been reviewed.

A cosmological constant is a famous part of Einstein's General Relativity theory, and refers to an arbitrary constant that is present in all related field equations.

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The question for theorists is: Has the growth of that cosmic yardstick accelerated steadily, in accordance with a cosmological constant, or does the acceleration vary over time?

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One is that dark energy is a cosmological constant, an unchanging property of space, which would mean that the universe would continue to expand indefinitely, sweeping far-off objects forever beyond our local point of view.

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One solution assumes dark energy isn’t a cosmological constant, but is due to some kind of new physics.

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In a Universe explained by Einstein's theory with a cosmological constant, black holes are immersed in a cosmological accelerated background.

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