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  • About
  • The Global ETD Search service is a free service for researchers to find electronic theses and dissertations. This service is provided by the Networked Digital Library of Theses and Dissertations.
    Our metadata is collected from universities around the world. If you manage a university/consortium/country archive and want to be added, details can be found on the NDLTD website.
1

Variáveis de contorno e loop de Wilson para uma classe de espaços-tempo

Santos, Edinelson Pereira dos 25 November 2011 (has links)
Submitted by Vasti Diniz (vastijpa@hotmail.com) on 2017-09-13T12:46:00Z No. of bitstreams: 1 aquivototal.pdf: 1083129 bytes, checksum: c7786a11a4d811fd716d27cf8c82948d (MD5) / Made available in DSpace on 2017-09-13T12:46:00Z (GMT). No. of bitstreams: 1 aquivototal.pdf: 1083129 bytes, checksum: c7786a11a4d811fd716d27cf8c82948d (MD5) Previous issue date: 2011-11-25 / Coordenação de Aperfeiçoamento de Pessoal de Nível Superior - CAPES / In thiswork,weinvestigateaclassofspace-timesbycalculatingtheloopvariables for differentcurves,intheparticularcasewherethepathstakenareclosed(circles),we obtain theso-calledholonomytransformations,fromwhichthetraceprovidesthematrix obtained intheWilsonloopgravitational.Firstwediscussthecasewherethegravita- tional fieldisgeneratedbyacylindricalshell,withoutrotation,intheapproximationof weak field.Thenwestudythespace-timesofGödelandFriedman-Robertson-Walker.We also investigatethespace-timesgeneratedbyacosmicstringwithinternalstructure.Fi- nally wediscusstheKottlerspace-timeandsomemodelsofwormholes.Tocalculatethe loop variablesweusetheperturbationexpansiontechnique,whichwecall perturbative method, andtechniquethroughtheLorentztransformationoflocalcoordinates,which we callthe exact method. Theobtainedresultsshowusthewaythesecontourvariables contain informationsrelatedtothegeometricalandtopologicalpropertiesofeachoneof these space-times. / Neste trabalho,investigamosumaclassedeespaços-tempoatravésdocálculodasva- riáveis decontornoparadiferentescurvas,quenocasoparticular,emqueoscaminhosto- mados sãofechados(círculos),obtêm-seasdenominadastransformaçõesdeholonomias, do qualotraçodamatrizobtidanosforneceoloopdeWilsongravitacional.Primeiro abordamos ocasoemqueocampogravitacionalégeradoporumacascacilíndrica,sem rotação,naaproximaçãodecampofraco.Emseguida,estudamososespaços-tempode Gödel eodeFriedman-Robertson-Walker.Tambéminvestigamosocenáriogeradopor uma cordacósmicacomestruturainterna.Porfim,abordamosoespaço-tempodeKöttle e algunsmodelosdewormholes.Paraocálculodasvariáveisdecontornoutilizamosa técnica daexpansãoperturbativa,oqualdenominamosde método perturbativo, eatéc- nica viatransformaçãodecoordenadasdeLorentzlocal,oqualdenominamosde método exato. Osresultadosnosmostramdequemaneiraessasvariáveisdecontornodetectam as característicasgeométricasetopológicasdecadaumdessesespaços-tempo.

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