A five-parameter class of solutions to the vacuum Einstein equations
We present a new five-parameter class of Ricci-flat solutions in four dimensions with Euclidean signature. The solution is asymptotically locally flat (ALF), and contains a finite asymptotic NUT charge. When this charge is sent to infinity, the solution becomes asymptotically locally Euclidean (ALE)...
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ftdatacite:10.48550/arxiv.1504.01235 2023-05-15T17:39:53+02:00 A five-parameter class of solutions to the vacuum Einstein equations Chen, Yu Teo, Edward 2015 https://dx.doi.org/10.48550/arxiv.1504.01235 https://arxiv.org/abs/1504.01235 unknown arXiv https://dx.doi.org/10.1103/physrevd.91.124005 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ General Relativity and Quantum Cosmology gr-qc FOS Physical sciences article-journal Article ScholarlyArticle Text 2015 ftdatacite https://doi.org/10.48550/arxiv.1504.01235 https://doi.org/10.1103/physrevd.91.124005 2022-04-01T12:11:25Z We present a new five-parameter class of Ricci-flat solutions in four dimensions with Euclidean signature. The solution is asymptotically locally flat (ALF), and contains a finite asymptotic NUT charge. When this charge is sent to infinity, the solution becomes asymptotically locally Euclidean (ALE), and one in fact obtains the Ricci-flat Plebanski-Demianski solution. The solution we have found can thus be regarded as an ALF generalisation of the latter solution. We also show that it can be interpreted as a system consisting of two touching Kerr-NUTs: the south pole of one Kerr-NUT touches the north pole of the other. The total NUT charge of such a system is then identified with the asymptotic NUT charge. Setting the asymptotic NUT charge to zero gives a four-parameter asymptotically flat (AF) solution, and contained within this subclass is the completely regular two-parameter AF instanton previously discovered by the present authors. Various other limits are also discussed, including that of the triple-collinearly-centered Gibbons-Hawking solution, and an ALF generalisation of the C-metric. : 33 pages, 4 figures, LaTeX Text North Pole South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole North Pole Kerr ENVELOPE(65.633,65.633,-70.433,-70.433) Alf ENVELOPE(-86.117,-86.117,-77.917,-77.917) |
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DataCite Metadata Store (German National Library of Science and Technology) |
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General Relativity and Quantum Cosmology gr-qc FOS Physical sciences |
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General Relativity and Quantum Cosmology gr-qc FOS Physical sciences Chen, Yu Teo, Edward A five-parameter class of solutions to the vacuum Einstein equations |
topic_facet |
General Relativity and Quantum Cosmology gr-qc FOS Physical sciences |
description |
We present a new five-parameter class of Ricci-flat solutions in four dimensions with Euclidean signature. The solution is asymptotically locally flat (ALF), and contains a finite asymptotic NUT charge. When this charge is sent to infinity, the solution becomes asymptotically locally Euclidean (ALE), and one in fact obtains the Ricci-flat Plebanski-Demianski solution. The solution we have found can thus be regarded as an ALF generalisation of the latter solution. We also show that it can be interpreted as a system consisting of two touching Kerr-NUTs: the south pole of one Kerr-NUT touches the north pole of the other. The total NUT charge of such a system is then identified with the asymptotic NUT charge. Setting the asymptotic NUT charge to zero gives a four-parameter asymptotically flat (AF) solution, and contained within this subclass is the completely regular two-parameter AF instanton previously discovered by the present authors. Various other limits are also discussed, including that of the triple-collinearly-centered Gibbons-Hawking solution, and an ALF generalisation of the C-metric. : 33 pages, 4 figures, LaTeX |
format |
Text |
author |
Chen, Yu Teo, Edward |
author_facet |
Chen, Yu Teo, Edward |
author_sort |
Chen, Yu |
title |
A five-parameter class of solutions to the vacuum Einstein equations |
title_short |
A five-parameter class of solutions to the vacuum Einstein equations |
title_full |
A five-parameter class of solutions to the vacuum Einstein equations |
title_fullStr |
A five-parameter class of solutions to the vacuum Einstein equations |
title_full_unstemmed |
A five-parameter class of solutions to the vacuum Einstein equations |
title_sort |
five-parameter class of solutions to the vacuum einstein equations |
publisher |
arXiv |
publishDate |
2015 |
url |
https://dx.doi.org/10.48550/arxiv.1504.01235 https://arxiv.org/abs/1504.01235 |
long_lat |
ENVELOPE(65.633,65.633,-70.433,-70.433) ENVELOPE(-86.117,-86.117,-77.917,-77.917) |
geographic |
South Pole North Pole Kerr Alf |
geographic_facet |
South Pole North Pole Kerr Alf |
genre |
North Pole South pole |
genre_facet |
North Pole South pole |
op_relation |
https://dx.doi.org/10.1103/physrevd.91.124005 |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.1504.01235 https://doi.org/10.1103/physrevd.91.124005 |
_version_ |
1766140658229182464 |