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We present a new signature by which to one could potentially discriminate between a spectrum of gravitational radiation generated by a self-ordering scalar field vs that of inflation, specifically a comparison of the magnitude of a flat spectrum at frequencies probed by future direct detection experiments to the magnitude of a possible polarization signal in the Cosmic Microwave Background (CMB) radiation.
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D. Baumann and M. Zaldarriaga, JCAP 0906:013 (2009)
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Fenu, E. , Figueroa, D. , Durrer, R. , Garcia-Bellido, J., JCAP 10 005 (2009); arXiv:0908.0425
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