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We construct a class of single small field models of inflation that can predict, contrary to popular wisdom, an observable gravitational wave signal in the cosmic microwave background anisotropies.
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D. H. Lyth, “What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?,” Phys. Rev. Lett. 78
1997
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D. H. Lyth and A. Riotto, “Particle physics models of inflation and the cosmological density perturbation,” Phys. Rept. 314
1999
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G. German, G. G. Ross and S. Sarkar, “Implementing quadratic supergravity inflation,” Phys. Lett. B 469
2001
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R. Brustein, S. P. De Alwis and E. G. Novak, “Inflationary cosmology in the central region of string / M-theory moduli space,” Phys. Rev. D 68
2003
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J. M. Maldacena, “Non-Gaussian features of primordial fluctuations in single field inflationary models,” JHEP 0305
2003
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P. Hunt and S. Sarkar, “Multiple inflation and the WMAP ’glitches’,” Phys. Rev. D 70
2004
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M. Tegmark et al
2006
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R. Easther and H. Peiris, “Implications of a running spectral index for slow roll inflation,” JCAP 0609
2006
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2007
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L. McAllister and E. Silverstein, “String Cosmology: A Review,” Gen. Rel. Grav. 40
2008
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R. Kallosh, “On Inflation in String Theory,” Lect. Notes Phys. 738
2008
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2008
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2009
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2008
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2009
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[Planck Collaboration], “Planck: The scientific programme,” arXiv:astro-ph/0604069
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2009
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S. Weinberg, “Non-Gaussian Correlations Outside the Horizon,” Phys. Rev. D 78
2009
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2010
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