The effect of the cosmological constant on background gravitational waves

Details The effect of the cosmological constant on background gravitational waves The effect of the cosmological constant on background gravitational waves

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001cqgra..18.5211h&link_type=abstract

Classical and Quantum Gravity, Volume 18, Issue 23, pp. 5211-5218 (2001).

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Scientific paper

The effect of a non-zero cosmological constant on the power spectrum of background gravitational waves is investigated. The power spectra of models with and without a non-zero cosmological constant are compared, and measurable differences between the models are identified. In particular, the power spectrum for non-zero cosmological constant is 0.3-0.6 times lower than the models with a zero constant for large-scale gravitational waves, yet identical at the super-horizon scale.

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