Geodesic Incompleteness and Partially Covariant Gravity

We study the issue of length renormalization in the context of fully covariant gravity theories as well as non-relativistic ones such as Hořava–Lifshitz gravity. The difference in their symmetry groups implies a relation among the lengths of paths in spacetime in the two types of theory. Provided th...

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Main Authors: Ignatios Antoniadis, Spiros Cotsakis
Format: Article
Language:English
Published: MDPI AG 2021-05-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/7/5/126
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author Ignatios Antoniadis
Spiros Cotsakis
author_facet Ignatios Antoniadis
Spiros Cotsakis
author_sort Ignatios Antoniadis
collection DOAJ
description We study the issue of length renormalization in the context of fully covariant gravity theories as well as non-relativistic ones such as Hořava–Lifshitz gravity. The difference in their symmetry groups implies a relation among the lengths of paths in spacetime in the two types of theory. Provided that certain asymptotic conditions hold, this relation allows us to transfer analytic criteria for the standard spacetime length to be finite and the Perelman length to be likewise finite, and therefore formulate conditions for geodesic incompleteness in partially covariant theories. We also discuss implications of this result for the issue of singularities in the context of such theories.
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spelling doaj.art-ccb88360cc7d4771888ce68aa1e9789d2023-11-21T18:11:35ZengMDPI AGUniverse2218-19972021-05-017512610.3390/universe7050126Geodesic Incompleteness and Partially Covariant GravityIgnatios Antoniadis0Spiros Cotsakis1Laboratoire de Physique Théorique et Hautes Energies—LPTHE, Sorbonne Université, CNRS 4 Place Jussieu, 75005 Paris, FranceInstitute of Gravitation and Cosmology, RUDN University, ul. Miklukho-Maklaya 6, 117198 Moscow, RussiaWe study the issue of length renormalization in the context of fully covariant gravity theories as well as non-relativistic ones such as Hořava–Lifshitz gravity. The difference in their symmetry groups implies a relation among the lengths of paths in spacetime in the two types of theory. Provided that certain asymptotic conditions hold, this relation allows us to transfer analytic criteria for the standard spacetime length to be finite and the Perelman length to be likewise finite, and therefore formulate conditions for geodesic incompleteness in partially covariant theories. We also discuss implications of this result for the issue of singularities in the context of such theories.https://www.mdpi.com/2218-1997/7/5/126Hořava–Lifshitz gravitygeodesic incompletenessgeometric flows
spellingShingle Ignatios Antoniadis
Spiros Cotsakis
Geodesic Incompleteness and Partially Covariant Gravity
Universe
Hořava–Lifshitz gravity
geodesic incompleteness
geometric flows
title Geodesic Incompleteness and Partially Covariant Gravity
title_full Geodesic Incompleteness and Partially Covariant Gravity
title_fullStr Geodesic Incompleteness and Partially Covariant Gravity
title_full_unstemmed Geodesic Incompleteness and Partially Covariant Gravity
title_short Geodesic Incompleteness and Partially Covariant Gravity
title_sort geodesic incompleteness and partially covariant gravity
topic Hořava–Lifshitz gravity
geodesic incompleteness
geometric flows
url https://www.mdpi.com/2218-1997/7/5/126
work_keys_str_mv AT ignatiosantoniadis geodesicincompletenessandpartiallycovariantgravity
AT spiroscotsakis geodesicincompletenessandpartiallycovariantgravity