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We investigate to which extent and under which circumstances false vacuum energy ($V_0$) dominated slow-roll inflation is compatible with a large tensor-to-scalar ratio $r = O(0.1)$, as indicated by the recent BICEP2 measurement.
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2009
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2010
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C. Dvorkin and W. Hu, Generalized Slow Roll for Large Power Spectrum Features
2010
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A. Mazumdar and J. Rocher, Particle physics models of inflation and curvaton scenarios
2011
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2012
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2012
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2013
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2013
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2011
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L. Senatore, E. Silverstein and M. Zaldarriaga, New Sources of Gravitational Waves during Inflation
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A. Moss and L. Pogosian, Did BICEP2 see vector modes? First B-mode constraints on cosmic defects
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Cited in the paper.
2014
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