Holography for Cosmology

R. Jackiw and S. Templeton, Phys. Rev. D23

1981

Earlier work this paper cites.

D. S. Salopek and J. R. Bond, Phys. Rev. D42

1990

Earlier work this paper cites.

M. Cvetic and H. H. Soleng, Phys. Rev. D51

1995

Earlier work this paper cites.

A. Kosowsky and M. Turner, Phys. Rev. D52

1995

Earlier work this paper cites.

S. de Haro, S. N. Solodukhin and K. Skenderis, Commun. Math. Phys. 217

2001

Earlier work this paper cites.

E. Komatsu and D. N. Spergel, Phys. Rev. D63

2001

Cited alongside, same era.

K.Skenderis, Class. Quant. Grav. 19

2002

Cited alongside, same era.

J. Maldacena, JHEP 05

2003

Cited alongside, same era.

I. Papadimitriou and K. Skenderis, JHEP 10

2004

Cited alongside, same era.

K. Skenderis and P. K. Townsend, Phys. Rev. Lett. 96

2007

Cited alongside, same era.

This era should then be followed by a hot big bang cosmology, as in standard discussions. Here we only discuss the very early universe, i.e.,

Cited in the paper.

P. McFadden and K. Skenderis, to appear

Cited in the paper.

Super-renormalizable theories have infrared divergences, but large N N resummation leads to well-defined expressions with g YM 2 g_{\mathrm{YM}}^{2} effectively playing the role of an infrared regulator. The exact amplitudes are nonanalytic functions of the coupling constant [ 17 ] . Note that our analytic continuation to pseudo-QFT does not involve the coupling constant

Cited in the paper.

E. A. Bergshoeff, J. Hartong, A. Ploegh, J. Rosseel and D. van den Bleeken, JHEP 07

Original

2007

Later among the works it cites.

P. McFadden and K. Skenderis, arxiv:1001.2007

Original

2007

Later among the works it cites.

K. Skenderis and B. C. van Rees, Phys. Rev. Lett. 101

Original

2008

Later among the works it cites.

I. Kanitscheider, K. Skenderis and M. Taylor, JHEP 09

Original

2008

Later among the works it cites.

E. Komatsu et al. (WMAP), Astrophys. J. Suppl. 180

Original

2009

Closest in time.