Built on

A. A. Starobinsky, Phys.Lett. B91
1980
Earlier work this paper cites.
A. Linde, Physics Letters B 108
1982
Earlier work this paper cites.
A. Albrecht and P. J. Steinhardt, Phys. Rev. Lett. 48
1982
Earlier work this paper cites.
J. Bond, A. H. Jaffe, and L. Knox, Phys.Rev. D57
1998
Earlier work this paper cites.
C. Bennett et al. (WMAP Collaboration), Astrophys.J.Suppl. 148
2003
Earlier work this paper cites.
C. Burgess, J. M. Cline, F. Lemieux, and R. Holman, JHEP 0302
2003
Earlier work this paper cites.
C. R. Contaldi, M. Peloso, L. Kofman, and A. D. Linde, JCAP 0307
2003
Earlier work this paper cites.
J. M. Cline, P. Crotty, and J. Lesgourgues, JCAP 0309
2003
Earlier work this paper cites.
M. Bastero-Gil, K. Freese, and L. Mersini-Houghton, Phys.Rev. D68
2003
Earlier work this paper cites.
S. Shankaranarayanan and L. Sriramkumar, 38(2004), arXiv:hep-th/0410072 [hep-th]
2004
Earlier work this paper cites.

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2013

Power Suppression at Large Scales in String Inflation

Cicoli, Michele, Downes, Sean, Dutta, Bhaskar

Understand

We study a possible origin of the anomalous suppression of the power spectrum at large angular scales in the cosmic microwave background within the framework of explicit string inflationary models where inflation is driven by a closed string modulus parameterizing the size of the extra dimensions.

In this class of models the apparent power loss at large scales is caused by the background dynamics which involves a sharp transition from a fast-roll power law phase to a period of Starobinsky-like slow-roll inflation.
An interesting feature of this class of string inflationary models is that the number of e-foldings of inflation is inversely proportional to the string coupling to a positive power.
Therefore once the string coupling is tuned to small values in order to trust string perturbation theory, enough e-foldings of inflation are automatically obtained without the need of extra tuning.

Built on

A. A. Starobinsky, Phys.Lett. B91
1980
Earlier work this paper cites.
A. Linde, Physics Letters B 108
1982
Earlier work this paper cites.
A. Albrecht and P. J. Steinhardt, Phys. Rev. Lett. 48
1982
Earlier work this paper cites.
J. Bond, A. H. Jaffe, and L. Knox, Phys.Rev. D57
1998
Earlier work this paper cites.
C. Bennett et al. (WMAP Collaboration), Astrophys.J.Suppl. 148
2003
Earlier work this paper cites.
C. Burgess, J. M. Cline, F. Lemieux, and R. Holman, JHEP 0302
2003
Earlier work this paper cites.
C. R. Contaldi, M. Peloso, L. Kofman, and A. D. Linde, JCAP 0307
2003
Earlier work this paper cites.
J. M. Cline, P. Crotty, and J. Lesgourgues, JCAP 0309
2003
Earlier work this paper cites.
M. Bastero-Gil, K. Freese, and L. Mersini-Houghton, Phys.Rev. D68
2003
Earlier work this paper cites.
S. Shankaranarayanan and L. Sriramkumar, 38(2004), arXiv:hep-th/0410072 [hep-th]
2004
Earlier work this paper cites.