2019-02-13T16:14:44Z
2019-02-13T16:14:44Z
2016-10-18
2019-02-13T16:14:44Z
It is well known that, in single clock inflation, the curvature perturbation is constant in time on superhorizon scales. In the standard bulk description this follows quite simply from the local conservation of the energy momentum tensor in the bulk. On the other hand, in a holographic description, the constancy of the curvature perturbation must be related to the properties of the RG flow in the boundary theory. Here, we show that, in single clock holographic inflation, the time independence of correlators of follows from the absence of the anomolous dimension of the energy momentum tensor in the boundary theory, and from the so-called consistency relations for vertex functions with a soft leg.
Article
Published version
English
Institute of Physics (IOP)
Reproducció del document publicat a: https://doi.org/10.1088/1475-7516/2016/10/030
Journal of Cosmology and Astroparticle Physics, 2016, vol. 2016, num. 030
https://doi.org/10.1088/1475-7516/2016/10/030
cc-by (c) Garriga Torres, Jaume et al., 2016
http://creativecommons.org/licenses/by/3.0/es