Numerical relativity investigation of the effects of gravitational waves on the inhomogeneity of the universe

Abstract We numerically integrate the Einstein’s equations for a spatially flat Friedmann–Lemaire–Robertson–Walker (FLRW) background spacetime with a spatial curvature perturbation and evolving primordial tensor perturbations using the Einstein Toolkit. We find that although the primordial tensor pe...

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Main Author: Ke Wang
Format: Article
Language:English
Published: SpringerOpen 2018-08-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-018-6103-7
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author Ke Wang
author_facet Ke Wang
author_sort Ke Wang
collection DOAJ
description Abstract We numerically integrate the Einstein’s equations for a spatially flat Friedmann–Lemaire–Robertson–Walker (FLRW) background spacetime with a spatial curvature perturbation and evolving primordial tensor perturbations using the Einstein Toolkit. We find that although the primordial tensor perturbation does not play an important role in the evolution of the overdensity produced by the scalar perturbation, there is an obvious imprint left by the primordial tensor perturbation on the distribution of the fractional density perturbation in the nonlinear region. This imprint may be a possible probe of a gravitational waves background in the future.
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spelling doaj.art-9659ad08b4784ed69b9948a3b25363e12022-12-21T23:55:32ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522018-08-017881710.1140/epjc/s10052-018-6103-7Numerical relativity investigation of the effects of gravitational waves on the inhomogeneity of the universeKe Wang0National Astronomical Observatories, Chinese Academy of SciencesAbstract We numerically integrate the Einstein’s equations for a spatially flat Friedmann–Lemaire–Robertson–Walker (FLRW) background spacetime with a spatial curvature perturbation and evolving primordial tensor perturbations using the Einstein Toolkit. We find that although the primordial tensor perturbation does not play an important role in the evolution of the overdensity produced by the scalar perturbation, there is an obvious imprint left by the primordial tensor perturbation on the distribution of the fractional density perturbation in the nonlinear region. This imprint may be a possible probe of a gravitational waves background in the future.http://link.springer.com/article/10.1140/epjc/s10052-018-6103-7
spellingShingle Ke Wang
Numerical relativity investigation of the effects of gravitational waves on the inhomogeneity of the universe
European Physical Journal C: Particles and Fields
title Numerical relativity investigation of the effects of gravitational waves on the inhomogeneity of the universe
title_full Numerical relativity investigation of the effects of gravitational waves on the inhomogeneity of the universe
title_fullStr Numerical relativity investigation of the effects of gravitational waves on the inhomogeneity of the universe
title_full_unstemmed Numerical relativity investigation of the effects of gravitational waves on the inhomogeneity of the universe
title_short Numerical relativity investigation of the effects of gravitational waves on the inhomogeneity of the universe
title_sort numerical relativity investigation of the effects of gravitational waves on the inhomogeneity of the universe
url http://link.springer.com/article/10.1140/epjc/s10052-018-6103-7
work_keys_str_mv AT kewang numericalrelativityinvestigationoftheeffectsofgravitationalwavesontheinhomogeneityoftheuniverse