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B. S. DeWitt and R. W. Brehme, Annals Phys. 9
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A. G. Riess et al
1999
Earlier work this paper cites.
S. Deser, Phys. Lett. B479
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Earlier work this paper cites.

Similar

N. C. Tsamis and R. P. Woodard, Nucl. Phys. B474
2005
Cited alongside, same era.
Y. Wang and P. Mukherjee, Astrophys. J. 650
2007
Cited alongside, same era.
N. C. Tsamis and R. P. Woodard, “Primordial Density Perturbations and Reheating from Gravity,” (preprint in preparation)
Cited in the paper.
S. Park and R. P. Woodard, arXiv:
Cited in the paper.

Then

S. Deser and R. P. Woodard, Phys. Rev. Lett. 99
2007
Later among the works it cites.
N. C. Tsamis and R. P. Woodard, Phys. Rev. D80
2009
Later among the works it cites.

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2010

Post-Inflationary Evolution via Gravitation

Tsamis, N. C., Woodard, R. P.

Understand

We study a class of non-local, purely gravitational models which have the correct structure to reproduce the leading infrared logarithms of quantum gravitational back-reaction during the inflationary regime.

These models end inflation in a distinctive phase of oscillations with slight and short violations of the weak energy condition and should, when coupled to matter, lead to rapid reheating.
By elaborating this class of models we exhibit one that has the same behaviour during inflation, goes quiescent until the onset of matter domination, and induces a small, positive cosmological constant of about the right size thereafter.