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Though simple inflationary models describe the CMB well, their corrections are often plagued by infrared effects that obstruct a reliable calculation of late-time behaviour.
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For implications for the solar interior and uncertainties in oscillation measurements see: C. P. Burgess, N. S. Dzhalilov, M. Maltoni, T. I. Rashba, V. B. Semikoz, M. A. Tortola and J. W. F. Valle, “Cornering solar radiative zone fluctuations with KamLAND and SNO salt,” JCAP 0401
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N. Afshordi and R. H. Brandenberger, “Super-Hubble nonlinear perturbations during inflation,” Phys. Rev. D 63
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D. Seery, “Infrared effects in inflationary correlation functions,” Class. Quant. Grav. 27
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2013
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T. Prokopec, “Late time solution for interacting scalar in accelerating spaces,” JCAP 1511
2015
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V. Vennin and A. A. Starobinsky, “Correlation Functions in Stochastic Inflation,” Eur. Phys. J. C 75
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2015
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