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deceleration parameter


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(q)

A figure that describes the slowing-down of the expansion of the Universe. In a Friedmann universe, the deceleration parameter is simply half the density parameter, Ω. A value of q greater than 0.5 indicates that the expansion is decelerating quickly enough for the Universe eventually to collapse. A value less than 0.5 indicates that the expansion will continue for ever. In models with a cosmological constant, q can even be negative, indicating an accelerated expansion, as in the inflationary universe.

Subjects: Astronomy and Astrophysics.


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