The Erez–Rosen Solution Versus the Hartle–Thorne Solution

In this work, we investigate the correspondence between the Erez−Rosen and Hartle−Thorne solutions. We explicitly show how to establish the relationship and find the coordinate transformations between the two metrics. For this purpose the two metrics must have the same approximat...

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Main Authors: Kuantay Boshkayev, Hernando Quevedo, Gulmira Nurbakyt, Algis Malybayev, Ainur Urazalina
Format: Article
Language:English
Published: MDPI AG 2019-10-01
Series:Symmetry
Subjects:
Online Access:https://www.mdpi.com/2073-8994/11/10/1324
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spelling doaj-d7972a6db8c746f8a07235d62419494d2020-11-25T01:56:45ZengMDPI AGSymmetry2073-89942019-10-011110132410.3390/sym11101324sym11101324The Erez–Rosen Solution Versus the Hartle–Thorne SolutionKuantay Boshkayev0Hernando Quevedo1Gulmira Nurbakyt2Algis Malybayev3Ainur Urazalina4National Nanotechnology Laboratory of Open Type, Department of Theoretical and Nuclear Physics, Al-Farabi Kazakh National University, Almaty 050040, KazakhstanNational Nanotechnology Laboratory of Open Type, Department of Theoretical and Nuclear Physics, Al-Farabi Kazakh National University, Almaty 050040, KazakhstanNational Nanotechnology Laboratory of Open Type, Department of Theoretical and Nuclear Physics, Al-Farabi Kazakh National University, Almaty 050040, KazakhstanNational Nanotechnology Laboratory of Open Type, Department of Theoretical and Nuclear Physics, Al-Farabi Kazakh National University, Almaty 050040, KazakhstanNational Nanotechnology Laboratory of Open Type, Department of Theoretical and Nuclear Physics, Al-Farabi Kazakh National University, Almaty 050040, KazakhstanIn this work, we investigate the correspondence between the Erez&#8722;Rosen and Hartle&#8722;Thorne solutions. We explicitly show how to establish the relationship and find the coordinate transformations between the two metrics. For this purpose the two metrics must have the same approximation and describe the gravitational field of static objects. Since both the Erez&#8722;Rosen and the Hartle&#8722;Thorne solutions are particular solutions of a more general solution, the Zipoy&#8722;Voorhees transformation is applied to the exact Erez&#8722;Rosen metric in order to obtain a generalized solution in terms of the Zipoy&#8722;Voorhees parameter <inline-formula> <math display="inline"> <semantics> <mrow> <mi>&#948;</mi> <mo>=</mo> <mn>1</mn> <mo>+</mo> <mi>s</mi> <mi>q</mi> </mrow> </semantics> </math> </inline-formula>. The Geroch&#8722;Hansen multipole moments of the generalized Erez&#8722;Rosen metric are calculated to find the definition of the total mass and quadrupole moment in terms of the mass <i>m</i>, quadrupole <i>q</i> and Zipoy&#8722;Voorhees <inline-formula> <math display="inline"> <semantics> <mi>&#948;</mi> </semantics> </math> </inline-formula> parameters. The coordinate transformations between the metrics are found in the approximation of &#8764;q. It is shown that the Zipoy&#8722;Voorhees parameter is equal to <inline-formula> <math display="inline"> <semantics> <mrow> <mi>&#948;</mi> <mo>=</mo> <mn>1</mn> <mo>&#8722;</mo> <mi>q</mi> </mrow> </semantics> </math> </inline-formula> with <inline-formula> <math display="inline"> <semantics> <mrow> <mi>s</mi> <mo>=</mo> <mo>&#8722;</mo> <mn>1</mn> </mrow> </semantics> </math> </inline-formula>. This result is in agreement with previous results in the literature.https://www.mdpi.com/2073-8994/11/10/1324vacuum solutionsquadrupole momentcoordinate transformations
collection DOAJ
language English
format Article
sources DOAJ
author Kuantay Boshkayev
Hernando Quevedo
Gulmira Nurbakyt
Algis Malybayev
Ainur Urazalina
spellingShingle Kuantay Boshkayev
Hernando Quevedo
Gulmira Nurbakyt
Algis Malybayev
Ainur Urazalina
The Erez–Rosen Solution Versus the Hartle–Thorne Solution
Symmetry
vacuum solutions
quadrupole moment
coordinate transformations
author_facet Kuantay Boshkayev
Hernando Quevedo
Gulmira Nurbakyt
Algis Malybayev
Ainur Urazalina
author_sort Kuantay Boshkayev
title The Erez–Rosen Solution Versus the Hartle–Thorne Solution
title_short The Erez–Rosen Solution Versus the Hartle–Thorne Solution
title_full The Erez–Rosen Solution Versus the Hartle–Thorne Solution
title_fullStr The Erez–Rosen Solution Versus the Hartle–Thorne Solution
title_full_unstemmed The Erez–Rosen Solution Versus the Hartle–Thorne Solution
title_sort erez–rosen solution versus the hartle–thorne solution
publisher MDPI AG
series Symmetry
issn 2073-8994
publishDate 2019-10-01
description In this work, we investigate the correspondence between the Erez&#8722;Rosen and Hartle&#8722;Thorne solutions. We explicitly show how to establish the relationship and find the coordinate transformations between the two metrics. For this purpose the two metrics must have the same approximation and describe the gravitational field of static objects. Since both the Erez&#8722;Rosen and the Hartle&#8722;Thorne solutions are particular solutions of a more general solution, the Zipoy&#8722;Voorhees transformation is applied to the exact Erez&#8722;Rosen metric in order to obtain a generalized solution in terms of the Zipoy&#8722;Voorhees parameter <inline-formula> <math display="inline"> <semantics> <mrow> <mi>&#948;</mi> <mo>=</mo> <mn>1</mn> <mo>+</mo> <mi>s</mi> <mi>q</mi> </mrow> </semantics> </math> </inline-formula>. The Geroch&#8722;Hansen multipole moments of the generalized Erez&#8722;Rosen metric are calculated to find the definition of the total mass and quadrupole moment in terms of the mass <i>m</i>, quadrupole <i>q</i> and Zipoy&#8722;Voorhees <inline-formula> <math display="inline"> <semantics> <mi>&#948;</mi> </semantics> </math> </inline-formula> parameters. The coordinate transformations between the metrics are found in the approximation of &#8764;q. It is shown that the Zipoy&#8722;Voorhees parameter is equal to <inline-formula> <math display="inline"> <semantics> <mrow> <mi>&#948;</mi> <mo>=</mo> <mn>1</mn> <mo>&#8722;</mo> <mi>q</mi> </mrow> </semantics> </math> </inline-formula> with <inline-formula> <math display="inline"> <semantics> <mrow> <mi>s</mi> <mo>=</mo> <mo>&#8722;</mo> <mn>1</mn> </mrow> </semantics> </math> </inline-formula>. This result is in agreement with previous results in the literature.
topic vacuum solutions
quadrupole moment
coordinate transformations
url https://www.mdpi.com/2073-8994/11/10/1324
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