Holographic No-Boundary Measure
Thomas Hertog, James Hartle
TL;DR
The paper shows that the complex saddle points of the no-boundary wave function with a positive cosmological constant and a positive scalar potential admit a representation in which the interior geometry is a regular Euclidean AdS domain wall smoothly transitioning to a Lorentzian inflationary de Sitter universe. The AdS portion regularizes volume divergences via counterterms and supplies a characteristic phase, enabling a holographic reformulation in which the semiclassical NBWF is encoded by the partition function of a dual field theory on the final boundary (a relevant deformation of an AdS/CFT CFT). This leads to a concrete dS/CFT-like duality: the NBWF amplitudes for coarse-grained classical configurations are given by $e^{I^{reg}_{DW}}/Z_{QFT}$ with a boundary phase, and bulk time evolution corresponds to inverse RG flow in the boundary theory. The authors conjecture that this duality extends beyond leading order, offering a pathway to compute string and quantum corrections to the cosmological measure from the dual QFT, and to test holographic cosmology in a controlled setting.
Abstract
We show that the complex saddle points of the no-boundary wave function with a positive cosmological constant and a positive scalar potential have a representation in which the geometry consists of a regular Euclidean AdS domain wall that makes a smooth transition to a Lorentzian, inflationary universe that is asymptotically deSitter. The transition region between AdS and dS regulates the volume divergences of the AdS action and accounts for the phases that explain the classical behavior of the final configuration. This leads to a dual formulation in which the semiclassical no-boundary measure is given in terms of the partition function of field theories on the final boundary that are certain relevant deformations of the CFTs that occur in AdS/CFT. We conjecture that the resulting dS/CFT duality holds also beyond the leading order approximation.
