File:Extended VIIh.jpg
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Summary
The temperature patterns in the cosmic microwave background expected in a Bianchi VII universe which was close to isotropy at early times. Inflation could occur in such a universe, albeit with some fine tuning; it would, at first order, superimpose stochastic, isotropic fluctuations on top of this pattern. From Pontzen (2009), based on the dynamical analysis of Pontzen and Challinor (2010).
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 18:18, 30 May 2015 | | 1,802 × 1,158 (650 KB) | Andrew Pontzen (Talk | contribs) | The temperature patterns in the cosmic microwave background expected in a Bianchi VII universe which was close to isotropy at early times. From Pontzen (2009), based on the dynamical analysis of Pontzen and Challinor (2010). |
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