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2010

Hilltop Supernatural Inflation

Lin, Chia-Min

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In this talk, I will explain how to reduce the spectral index to be n_s=0.96 for supernatural inflation.

I will also show the constraint to the reheating temperature from Big Bang Nucleosynthesis of both thermal and non-thermal gravitino production.

Hilltop Supernatural Inflation · Around

Built on

M. Kawasaki, T. Moroi, Prog. Theor. Phys. 93
1995
Earlier work this paper cites.
L. Randall, M. Soljacic, A. H. Guth, Nucl. Phys. B472
1996
Earlier work this paper cites.
L. Boubekeur, D. .H. Lyth, JCAP 0507
2005
Earlier work this paper cites.

Similar

M. Kawasaki, F. Takahashi, T. T. Yanagida, Phys. Lett. B638
2006
Cited alongside, same era.
K. Kohri, C. -M. Lin, D. H. Lyth, JCAP 0712
Original
2007
Cited alongside, same era.
A. D. Linde, “Particle Physics and Inflationary Cosmology,” Chur, Switzerland: Harwood (1990) 362 p; D. H. Lyth and A. Riotto, Phys. Rept. 314
Original
2009
Cited alongside, same era.
E. Komatsu, K. M. Smith, J. Dunkley et al
Original
Cited in the paper.

Then

C. -M. Lin, K. Cheung, Phys. Rev. D79
Original
2009
Later among the works it cites.
K. Kohri, C. -M. Lin, JCAP 1011
Original
2010
Closest in time.
C. -M. Lin, K. Cheung, Mod. Phys. Lett. A25
Original
2010
Closest in time.

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