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The cosmic gravitational wave background is a relic of the Cosmic inflation, which 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]
[edit] See also
[edit] References
- ^ "Gravitational Wave Background". Retrieved on 2007-06-20.
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Gravitational wave observatories |
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| Ground-based (proposed) |
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| Space-based (planned and proposed) |
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| Data analysis |
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