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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Autor principal: Chimento, Luis Pascual
Publicado: 1997
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00222488_v38_n5_p2565_Chimento
http://hdl.handle.net/20.500.12110/paper_00222488_v38_n5_p2565_Chimento
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spelling paper:paper_00222488_v38_n5_p2565_Chimento2023-06-08T14:48:11Z Form invariance of differential equations in general relativity Chimento, Luis Pascual 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. 1997 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00222488_v38_n5_p2565_Chimento http://hdl.handle.net/20.500.12110/paper_00222488_v38_n5_p2565_Chimento
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (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.
author Chimento, Luis Pascual
spellingShingle Chimento, Luis Pascual
Form invariance of differential equations in general relativity
author_facet Chimento, Luis Pascual
author_sort Chimento, Luis Pascual
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 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00222488_v38_n5_p2565_Chimento
http://hdl.handle.net/20.500.12110/paper_00222488_v38_n5_p2565_Chimento
work_keys_str_mv AT chimentoluispascual forminvarianceofdifferentialequationsingeneralrelativity
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