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String Gas Cosmology: Challenging Inflation | Robert Brandenberger (#336)

Into the Impossible With Brian Keating

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How to Obtain an Early Universe Cosmology Without Scale Fields

Since you have a thermal state, we have thermal fluctuations. So there'll be no deviation from the Harrison's old average. Ah, now comes the fluctuations. We can compute the perturbations and we find that we get something that is roughly consistent with observations. And if we now go back to our string gas cosmology toy model, then we automatically get the tilt, get the deviation and we get this consistent relation. There's no cosmological constant. But I think I've answered your program. This is an attempt to obtain an early universe cosmology, which does not involve scale fields.

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