Form invariance of differential equations in general relativity
Einstein equations for several matter sources in Robertson-Walker and Bianchi I type metrics, are shown to reduce to a kind of second-order nonlinear ordinary differential equation ÿ + αf(y)ẏ + βf(y)(Latin small letter esh)f(y)dy + γf(y) = 0. Also, it appears in the generalized statistical mechanics...
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I28-R145-paper_00222488_v38_n5_p2565_Chimento_oai2024-08-16 Chimento, L.P. 1997 Einstein equations for several matter sources in Robertson-Walker and Bianchi I type metrics, are shown to reduce to a kind of second-order nonlinear ordinary differential equation ÿ + αf(y)ẏ + βf(y)(Latin small letter esh)f(y)dy + γf(y) = 0. Also, it appears in the generalized statistical mechanics for the most interesting value q = -1. The invariant form of this equation is imposed and the corresponding nonlocal transformation is obtained. The linearization of that equation for any α, β, and γ is presented and for the important case f = byn + k with β = α2 (n + 1)/(n + 2)2 its explicit general solution is found. Moreover, the form invariance is applied to yield exact solutions of some other differential equations. © 1997 American Institute of Physics. Fil:Chimento, L.P. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. application/pdf http://hdl.handle.net/20.500.12110/paper_00222488_v38_n5_p2565_Chimento info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar J. Math. Phys. 1997;38(5):2565-2576 Form invariance of differential equations in general relativity info:eu-repo/semantics/article info:ar-repo/semantics/artículo info:eu-repo/semantics/publishedVersion https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_00222488_v38_n5_p2565_Chimento_oai |
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Universidad de Buenos Aires |
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I-28 |
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R-145 |
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Repositorio Digital de la Universidad de Buenos Aires (UBA) |
description |
Einstein equations for several matter sources in Robertson-Walker and Bianchi I type metrics, are shown to reduce to a kind of second-order nonlinear ordinary differential equation ÿ + αf(y)ẏ + βf(y)(Latin small letter esh)f(y)dy + γf(y) = 0. Also, it appears in the generalized statistical mechanics for the most interesting value q = -1. The invariant form of this equation is imposed and the corresponding nonlocal transformation is obtained. The linearization of that equation for any α, β, and γ is presented and for the important case f = byn + k with β = α2 (n + 1)/(n + 2)2 its explicit general solution is found. Moreover, the form invariance is applied to yield exact solutions of some other differential equations. © 1997 American Institute of Physics. |
format |
Artículo Artículo publishedVersion |
author |
Chimento, L.P. |
spellingShingle |
Chimento, L.P. Form invariance of differential equations in general relativity |
author_facet |
Chimento, L.P. |
author_sort |
Chimento, L.P. |
title |
Form invariance of differential equations in general relativity |
title_short |
Form invariance of differential equations in general relativity |
title_full |
Form invariance of differential equations in general relativity |
title_fullStr |
Form invariance of differential equations in general relativity |
title_full_unstemmed |
Form invariance of differential equations in general relativity |
title_sort |
form invariance of differential equations in general relativity |
publishDate |
1997 |
url |
http://hdl.handle.net/20.500.12110/paper_00222488_v38_n5_p2565_Chimento https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_00222488_v38_n5_p2565_Chimento_oai |
work_keys_str_mv |
AT chimentolp forminvarianceofdifferentialequationsingeneralrelativity |
_version_ |
1809356792191254528 |