Hodge-de Rham Laplacian and geometric criteria for gravitational waves

The curvature tensor \(\hat{R}\) of a manifold is called harmonic, if it obeys the condition \(\Delta^{\text{(HR)}}\hat{R}=0\), where \(\Delta^{\text{(HR)}}=DD^{\ast} + D^{\ast}D\) is the Hodge–deRham Laplacian. It is proved that all solutions of the Einstein equations in vacuum, as well as all sol...

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Main Authors: Olga V. Babourova, Boris N. Frolov
Format: Article
Language:English
Published: Peoples’ Friendship University of Russia (RUDN University) 2023-09-01
Series:Discrete and Continuous Models and Applied Computational Science
Subjects:
Online Access:https://journals.rudn.ru/miph/article/viewFile/35920/22462
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author Olga V. Babourova
Boris N. Frolov
author_facet Olga V. Babourova
Boris N. Frolov
author_sort Olga V. Babourova
collection DOAJ
description The curvature tensor \(\hat{R}\) of a manifold is called harmonic, if it obeys the condition \(\Delta^{\text{(HR)}}\hat{R}=0\), where \(\Delta^{\text{(HR)}}=DD^{\ast} + D^{\ast}D\) is the Hodge–deRham Laplacian. It is proved that all solutions of the Einstein equations in vacuum, as well as all solutions of the Einstein–Cartan theory in vacuum have a harmonic curvature. The statement that only solutions of Einstein’s equations of type \(N\) (describing gravitational radiation) are harmonic is refuted.
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spelling doaj.art-5658cf685fcc460896a93a45d8637e492023-09-18T12:29:16ZengPeoples’ Friendship University of Russia (RUDN University)Discrete and Continuous Models and Applied Computational Science2658-46702658-71492023-09-0131324224610.22363/2658-4670-2023-31-3-242-24621022Hodge-de Rham Laplacian and geometric criteria for gravitational wavesOlga V. Babourova0https://orcid.org/0000-0002-2527-5268Boris N. Frolov1https://orcid.org/0000-0002-8899-1894Moscow Automobile and Road Construction State Technical UniversityMoscow Pedagogical State UniversityThe curvature tensor \(\hat{R}\) of a manifold is called harmonic, if it obeys the condition \(\Delta^{\text{(HR)}}\hat{R}=0\), where \(\Delta^{\text{(HR)}}=DD^{\ast} + D^{\ast}D\) is the Hodge–deRham Laplacian. It is proved that all solutions of the Einstein equations in vacuum, as well as all solutions of the Einstein–Cartan theory in vacuum have a harmonic curvature. The statement that only solutions of Einstein’s equations of type \(N\) (describing gravitational radiation) are harmonic is refuted.https://journals.rudn.ru/miph/article/viewFile/35920/22462hodge-de rham laplacianharmonic curvature tensorharmonic solutions in vacuum of einstein equation and einstein-cartan theory equations
spellingShingle Olga V. Babourova
Boris N. Frolov
Hodge-de Rham Laplacian and geometric criteria for gravitational waves
Discrete and Continuous Models and Applied Computational Science
hodge-de rham laplacian
harmonic curvature tensor
harmonic solutions in vacuum of einstein equation and einstein-cartan theory equations
title Hodge-de Rham Laplacian and geometric criteria for gravitational waves
title_full Hodge-de Rham Laplacian and geometric criteria for gravitational waves
title_fullStr Hodge-de Rham Laplacian and geometric criteria for gravitational waves
title_full_unstemmed Hodge-de Rham Laplacian and geometric criteria for gravitational waves
title_short Hodge-de Rham Laplacian and geometric criteria for gravitational waves
title_sort hodge de rham laplacian and geometric criteria for gravitational waves
topic hodge-de rham laplacian
harmonic curvature tensor
harmonic solutions in vacuum of einstein equation and einstein-cartan theory equations
url https://journals.rudn.ru/miph/article/viewFile/35920/22462
work_keys_str_mv AT olgavbabourova hodgederhamlaplacianandgeometriccriteriaforgravitationalwaves
AT borisnfrolov hodgederhamlaplacianandgeometriccriteriaforgravitationalwaves