Physical instabilities and the phase of the Euclidean path integral

Fuente: arXiv
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Autori principali: Ivo, Victor, Maldacena, Juan, Sun, Zimo
Natura: Preprint
Pubblicazione: 2025
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author Ivo, Victor
Maldacena, Juan
Sun, Zimo
author_facet Ivo, Victor
Maldacena, Juan
Sun, Zimo
contents We compute the phase of the Euclidean gravity partition function on manifolds of the form $S^p \times M_q$. We find that the total phase is equal to the phase in pure gravity on $S^p$ times an extra phase that arises from negative mass squared fields that we obtain when we perform a Kaluza-Klein reduction to $S^p$. The latter can be matched to the phase expected for physical negative modes seen by a static path observer in $dS_p$. In the case of $S^p \times S^q$ the answer can be interpreted in terms of a computation in the static patch of $dS_p$ or $dS_q$. We also provide the phase when we have a product of many spheres. We clarify the procedure for determining the precise phase factor. We discuss some aspects of the interpretation of this phase.
format Preprint
id arxiv_https___arxiv_org_abs_2504_00920
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Physical instabilities and the phase of the Euclidean path integral
Ivo, Victor
Maldacena, Juan
Sun, Zimo
High Energy Physics - Theory
We compute the phase of the Euclidean gravity partition function on manifolds of the form $S^p \times M_q$. We find that the total phase is equal to the phase in pure gravity on $S^p$ times an extra phase that arises from negative mass squared fields that we obtain when we perform a Kaluza-Klein reduction to $S^p$. The latter can be matched to the phase expected for physical negative modes seen by a static path observer in $dS_p$. In the case of $S^p \times S^q$ the answer can be interpreted in terms of a computation in the static patch of $dS_p$ or $dS_q$. We also provide the phase when we have a product of many spheres. We clarify the procedure for determining the precise phase factor. We discuss some aspects of the interpretation of this phase.
title Physical instabilities and the phase of the Euclidean path integral
topic High Energy Physics - Theory
url https://arxiv.org/abs/2504.00920