{"title":"Similarity in the Arnowitt-Deser-Misner Mass from Brill and Teukolsky Initial Data Sets Beyond the Linear Approximation","authors":"R. F. Aranha, H. P. de Oliveira","doi":"arxiv-2409.04281","DOIUrl":null,"url":null,"abstract":"The two most common initial data for vacuum axisymmetric spacetimes are the\nBrill and Teukolsky gravitational waves. The subsequent numerical evolution of\nthese data exhibits distinct properties mainly associated with the critical\ngravitational collapse. A possible way of understanding these differences is\nfirst to look at the linear level, where the Brill waves have a multipolar\nstructure, while the Teukolsky waves have a quadrupolar structure. Despite\nbeing structurally distinct at the linear and nonlinear levels, we show that\nthese gravitational wave initial data share an unexpected similarity related to\nthe distribution of ADM mass as a function of the initial wave's amplitude.\nMore specifically, both configurations satisfy a nonextensive relation,\ncommonly seen in systems governed by long range interactions.","PeriodicalId":501041,"journal":{"name":"arXiv - PHYS - General Relativity and Quantum Cosmology","volume":"11 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - General Relativity and Quantum Cosmology","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.04281","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
The two most common initial data for vacuum axisymmetric spacetimes are the
Brill and Teukolsky gravitational waves. The subsequent numerical evolution of
these data exhibits distinct properties mainly associated with the critical
gravitational collapse. A possible way of understanding these differences is
first to look at the linear level, where the Brill waves have a multipolar
structure, while the Teukolsky waves have a quadrupolar structure. Despite
being structurally distinct at the linear and nonlinear levels, we show that
these gravitational wave initial data share an unexpected similarity related to
the distribution of ADM mass as a function of the initial wave's amplitude.
More specifically, both configurations satisfy a nonextensive relation,
commonly seen in systems governed by long range interactions.