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In page Hubble's law:

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However, in the standard Lambda-CDM model, q {\displaystyle q} will tend to −1 from above in the distant future as the cosmological constant becomes increasingly dominant over matter; this implies that H {\displaystyle H} will approach from above to a constant value of ≈ 57 {\displaystyle \approx 57} km/s/Mpc, and the scale factor of the universe will then grow exponentially in time.