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In this follow-up to our paper from 2005, we briefly discuss the implications of the apparent detection of B modes in the Cosmic Microwave Background for the issues raised in that paper.
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Earlier work this paper cites.
D. H. Lyth, “What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?,” Phys. Rev. Lett. 78
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Earlier work this paper cites.
B. Freivogel, M. Kleban, M. Rodriguez Martinez and L. Susskind, “Observational consequences of a landscape,” JHEP 0603
2006
Earlier work this paper cites.
N. Kaloper, A. Lawrence and L. Sorbo, “An Ignoble Approach to Large Field Inflation,” JCAP 1103
2008
Earlier work this paper cites.
J. March-Russell and F. Riva, “Signals of Inflation in a Friendly String Landscape,” JHEP 0607
2010
Cited alongside, same era.
2011
Cited alongside, same era.
M. Kleban and M. Schillo, “Spatial Curvature Falsifies Eternal Inflation,” JCAP 1206
2012
Cited alongside, same era.
A. H. Guth and Y. Nomura, “What can the observation of nonzero curvature tell us?,” Phys. Rev. D 86
2012
Cited alongside, same era.
Cited in the paper.
Cited in the paper.
Cited in the paper.
R. Bousso, D. Harlow, and L. Senatore, to appear
Cited in the paper.
F. G. Pedro and A. Westphal, “Low-l CMB Power Loss in String Inflation,” arXiv:1309.3413 [hep-th]
Cited in the paper.
Cited in the paper.
2013
Later among the works it cites.
2013
Later among the works it cites.
2013
Later among the works it cites.
2013
Later among the works it cites.
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