New regularization scheme for the wave function of the Universe in the Lorentzian path integral

The Lorentzian path integral for the wave function of the Universe is only conditionally convergent and thus requires a well-defined prescription. The Picard-Lefschetz approach ensures convergence through contour deformation, but it has been argued that this leads to unsuppressed perturbations due to relevant saddle points residing in the region <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"> <a:mrow> <a:mi>Im</a:mi> <a:mtext> </a:mtext> <a:mi>N</a:mi> <a:mo>&gt;</a:mo> <a:mn>0</a:mn> </a:mrow> </a:math> . As an alternative, we propose a simple regulator for the lapse integral in minisuperspace. Specifically, we impose the vanishing initial size of the Universe via a delta function, represented as a narrow Gaussian of width <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"> <c:mi>σ</c:mi> </c:math> , and take the limit <e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"> <e:mi>σ</e:mi> <e:mo stretchy="false">→</e:mo> <e:mn>0</e:mn> </e:math> only after performing the functional integrations. This regulator has a clear physical interpretation: it corresponds to a vanishingly small quantum uncertainty in the initial size of the Universe. For any fixed <h:math xmlns:h="http://www.w3.org/1998/Math/MathML" display="inline"> <h:mi>σ</h:mi> <h:mo>&gt;</h:mo> <h:mn>0</h:mn> </h:math> , the lapse integral is absolutely convergent along (or slightly below) the real axis, and no excursion into the region <j:math xmlns:j="http://www.w3.org/1998/Math/MathML" display="inline"> <j:mrow> <j:mi>Im</j:mi> <j:mtext> </j:mtext> <j:mi>N</j:mi> <j:mo>&gt;</j:mo> <j:mn>0</j:mn> </j:mrow> </j:math> is required. We further argue that the initial wave function for scalar and tensor perturbations should be incorporated in the Lorentzian path integral formalism, and we show that these perturbations are then appropriately suppressed. A purely Lorentzian path integral thus yields the tunneling wave function with suppressed perturbations. We also demonstrate that the Hartle-Hawking wave function can be reproduced by choosing a contour for the lapse integral extending from <l:math xmlns:l="http://www.w3.org/1998/Math/MathML" display="inline"> <l:mo>−</l:mo> <l:mi>∞</l:mi> </l:math> to <n:math xmlns:n="http://www.w3.org/1998/Math/MathML" display="inline"> <n:mo>+</n:mo> <n:mi>∞</n:mi> </n:math> that passes below the singularity near the origin.