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We test a class of holographic models for the very early universe against cosmological observations and find that they are competitive to the standard $\Lambda$CDM model of cosmology.
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J. B. Hartle, S. W. Hawking, and T. Hertog, (2012), arXiv:1205.3807 [hep-th]
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C. Corianò, L. Delle Rose, and M. Serino, JHEP 12
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2014
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P. A. R. Ade et al. (Planck), Astron. Astrophys. 571
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J. Garriga, K. Skenderis, and Y. Urakawa, JCAP 1501
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N. Kundu, A. Shukla, and S. P. Trivedi, JHEP 04
2015
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N. Kundu, A. Shukla, and S. P. Trivedi, JHEP 01
2016
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T. Hertog and E. van der Woerd, JCAP 1602
2016
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J. Garriga, Y. Urakawa, and F. Vernizzi, JCAP 1602
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J. Garriga and Y. Urakawa, (2016), arXiv:1606.04767 [hep-th]
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N. Afshordi, E. Gould, and K. Skenderis, (2016), to appear
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C. Corianò, L. Delle Rose, and K. Skenderis, (2016), to appear
2016
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R. Easther, R. Flauger, P. McFadden, and K. Skenderis, JCAP 1109
2040
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