Cosmic gravitational wave background

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The cosmic gravitational wave background is a relic of the Cosmic inflation that can be measured directly or indirectly by examining the polarization of the Cosmic microwave background radiation. It is the result of three things: inflationary expansion of space itself, reheating after inflation, and turbulent fluid mixing of matter and radiation. [1]

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References[edit]

  1. ^ "Gravitational Wave Background". Retrieved 2007-06-20.