<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-09-19T10:58:30Z</responseDate><request verb="GetRecord" identifier="oai:cora.ucc.ie:10468/527" metadataPrefix="dim">https://cora.ucc.ie/server/oai/request</request><GetRecord><record><header><identifier>oai:cora.ucc.ie:10468/527</identifier><datestamp>2023-04-04T07:10:41Z</datestamp><setSpec>com_10468_388</setSpec><setSpec>com_10468_5</setSpec><setSpec>com_10468_1</setSpec><setSpec>com_10468_224</setSpec><setSpec>col_10468_389</setSpec><setSpec>col_10468_140</setSpec><setSpec>col_10468_430</setSpec></header><metadata><dim:dim xmlns:dim="http://www.dspace.org/xmlns/dspace/dim" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://www.dspace.org/xmlns/dspace/dim http://www.dspace.org/schema/dim.xsd">
   <dim:field mdschema="dc" element="contributor" qualifier="advisor">Ó Murchadha, Niall</dim:field>
   <dim:field mdschema="dc" element="contributor" qualifier="author">Conboye, Rory P. A.</dim:field>
   <dim:field mdschema="dc" element="contributor" qualifier="funder" lang="en">Science Foundation Ireland</dim:field>
   <dim:field mdschema="dc" element="date" qualifier="accessioned">2012-02-21T11:38:56Z</dim:field>
   <dim:field mdschema="dc" element="date" qualifier="available">2012-02-21T11:38:56Z</dim:field>
   <dim:field mdschema="dc" element="date" qualifier="issued">2012-02</dim:field>
   <dim:field mdschema="dc" element="date" qualifier="submitted">2012-02-14</dim:field>
   <dim:field mdschema="dc" element="description" qualifier="abstract" lang="en">Transverse trace-free (TT) tensors play an important role in the initial conditions of numerical relativity, containing two of the component freedoms. Expressing a TT tensor entirely, by the choice of two scalar potentials, is not a trivial task however. Assuming the added condition of axial symmetry, expressions are given in both spherical and cylindrical coordinates, for TT tensors in flat space. A coordinate relation is then calculated between the scalar potentials of each coordinate system. This is extended to a non-flat space, though only one potential is found. The remaining equations are reduced to form a second order partial differential equation in two of the tensor components. With the axially symmetric flat space tensors, the choice of potentials giving Bowen-York conformal curvatures, are derived. A restriction is found for the potentials which ensure an axially symmetric TT tensor, which is regular at the origin, and conditions on the potentials, which give an axially symmetric TT tensor with a spherically symmetric scalar product, are also derived. A comparison is made of the extrinsic curvatures of the exact Kerr solution and numerical Bowen-York solution for axially symmetric black hole space-times. The Brill wave, believed to act as the difference between the Kerr and Bowen-York space-times, is also studied, with an approximate numerical solution found for a mass-factor, under different amplitudes of the metric.</dim:field>
   <dim:field mdschema="dc" element="description" qualifier="status" lang="en">Not peer reviewed</dim:field>
   <dim:field mdschema="dc" element="description" qualifier="version" lang="en">Accepted Version</dim:field>
   <dim:field mdschema="dc" element="format" qualifier="mimetype" lang="en">application/pdf</dim:field>
   <dim:field mdschema="dc" element="identifier" qualifier="citation" lang="en">Conboye, Rory P.A. 2012. Axial Symmetry and Transverse Trace-Free Tensors in Numerical Relativity. PhD Thesis, University College Cork.</dim:field>
   <dim:field mdschema="dc" element="identifier" qualifier="uri">https://hdl.handle.net/10468/527</dim:field>
   <dim:field mdschema="dc" element="language" qualifier="iso" lang="en">en</dim:field>
   <dim:field mdschema="dc" element="publisher" lang="en">University College Cork</dim:field>
   <dim:field mdschema="dc" element="rights" lang="en">©  2012, Rory Patrick Albert Conboye</dim:field>
   <dim:field mdschema="dc" element="rights" qualifier="uri" lang="en">http://creativecommons.org/licenses/by-nc-nd/3.0/</dim:field>
   <dim:field mdschema="dc" element="subject" lang="en">Numerical relativity</dim:field>
   <dim:field mdschema="dc" element="subject" lang="en">Initial value problem</dim:field>
   <dim:field mdschema="dc" element="subject" qualifier="lcsh" lang="en">Relativity (Physics)</dim:field>
   <dim:field mdschema="dc" element="subject" qualifier="lcsh" lang="en">Geometry, Differential</dim:field>
   <dim:field mdschema="dc" element="subject" qualifier="lcsh" lang="en">Mathematical physics</dim:field>
   <dim:field mdschema="dc" element="title" lang="en">Axial symmetry and transverse trace-free tensors in numerical relativity</dim:field>
   <dim:field mdschema="dc" element="type" lang="en">Doctoral thesis</dim:field>
   <dim:field mdschema="dc" element="type" qualifier="qualificationlevel" lang="en">Doctoral</dim:field>
   <dim:field mdschema="dc" element="type" qualifier="qualificationname" lang="en">PhD (Physics)</dim:field>info:eu-repo/semantics/openAccess</dim:dim></metadata></record></GetRecord></OAI-PMH>