Null Geodesic Congruences, Asymptotically-Flat Spacetimes and Their Physical Interpretation
- Autores
- Adamo, Timothy M.; Newman, Ezra T.; Kozameh, Carlos Nicolas
- Año de publicación
- 2012
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- A priori, there is nothing very special about shear-free or asymptotically shear-free null geodesic congruences. Surprisingly, however, they turn out to possess a large number of fascinating geometric properties and to be closely related, in the context of general relativity, to a variety of physically significant effects. It is the purpose of this paper to try to fully develop these issues. This work starts with a detailed exposition of the theory of shear-free and asymptotically shear-free null geodesic congruences, i.e., congruences with shear that vanishes at future conformal null infinity. A major portion of the exposition lies in the analysis of the space of regular shear-free and asymptotically shear-free null geodesic congruences. This analysis leads to the space of complex analytic curves in an auxiliary four-complex dimensional space, ℋ-space. They in turn play a dominant role in the applications. The applications center around the problem of extracting interior physical properties of an asymptotically-flat spacetime directly from the asymptotic gravitational (and Maxwell) field itself, in analogy with the determination of total charge by an integral over the Maxwell field at infinity or the identification of the interior mass (and its loss) by (Bondi’s) integrals of the Weyl tensor, also at infinity. More specifically, we will see that the asymptotically shear-free congruences lead us to an asymptotic definition of the center-of-mass and its equations of motion. This includes a kinematic meaning, in terms of the center-of-mass motion, for the Bondi three-momentum. In addition, we obtain insights into intrinsic spin and, in general, angular momentum, including an angular-momentum–conservation law with well-defined flux terms. When a Maxwell field is present, the asymptotically shear-free congruences allow us to determine/define at infinity a center-of-charge world line and intrinsic magnetic dipole moment.
Fil: Adamo, Timothy M.. University of Oxford; Reino Unido
Fil: Newman, Ezra T.. University of Pittsburgh; Estados Unidos
Fil: Kozameh, Carlos Nicolas. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Física Enrique Gaviola. Universidad Nacional de Córdoba. Instituto de Física Enrique Gaviola; Argentina - Materia
-
SHEAR FREE CONGRUENCES
CENTER OF MASS
ANGULAR MOMENTUM - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-nd/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/268630
Ver los metadatos del registro completo
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Null Geodesic Congruences, Asymptotically-Flat Spacetimes and Their Physical InterpretationAdamo, Timothy M.Newman, Ezra T.Kozameh, Carlos NicolasSHEAR FREE CONGRUENCESCENTER OF MASSANGULAR MOMENTUMhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1A priori, there is nothing very special about shear-free or asymptotically shear-free null geodesic congruences. Surprisingly, however, they turn out to possess a large number of fascinating geometric properties and to be closely related, in the context of general relativity, to a variety of physically significant effects. It is the purpose of this paper to try to fully develop these issues. This work starts with a detailed exposition of the theory of shear-free and asymptotically shear-free null geodesic congruences, i.e., congruences with shear that vanishes at future conformal null infinity. A major portion of the exposition lies in the analysis of the space of regular shear-free and asymptotically shear-free null geodesic congruences. This analysis leads to the space of complex analytic curves in an auxiliary four-complex dimensional space, ℋ-space. They in turn play a dominant role in the applications. The applications center around the problem of extracting interior physical properties of an asymptotically-flat spacetime directly from the asymptotic gravitational (and Maxwell) field itself, in analogy with the determination of total charge by an integral over the Maxwell field at infinity or the identification of the interior mass (and its loss) by (Bondi’s) integrals of the Weyl tensor, also at infinity. More specifically, we will see that the asymptotically shear-free congruences lead us to an asymptotic definition of the center-of-mass and its equations of motion. This includes a kinematic meaning, in terms of the center-of-mass motion, for the Bondi three-momentum. In addition, we obtain insights into intrinsic spin and, in general, angular momentum, including an angular-momentum–conservation law with well-defined flux terms. When a Maxwell field is present, the asymptotically shear-free congruences allow us to determine/define at infinity a center-of-charge world line and intrinsic magnetic dipole moment.Fil: Adamo, Timothy M.. University of Oxford; Reino UnidoFil: Newman, Ezra T.. University of Pittsburgh; Estados UnidosFil: Kozameh, Carlos Nicolas. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Física Enrique Gaviola. Universidad Nacional de Córdoba. Instituto de Física Enrique Gaviola; ArgentinaSpringer2012-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/268630Adamo, Timothy M.; Newman, Ezra T.; Kozameh, Carlos Nicolas; Null Geodesic Congruences, Asymptotically-Flat Spacetimes and Their Physical Interpretation; Springer; Living Reviews in Relativity; 15; 1; 1-2012; 1-921433-8351CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.12942/lrr-2012-1info:eu-repo/semantics/altIdentifier/doi/10.12942/lrr-2012-1info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-nd/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2026-02-26T10:02:43Zoai:ri.conicet.gov.ar:11336/268630instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982026-02-26 10:02:43.743CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
Null Geodesic Congruences, Asymptotically-Flat Spacetimes and Their Physical Interpretation |
| title |
Null Geodesic Congruences, Asymptotically-Flat Spacetimes and Their Physical Interpretation |
| spellingShingle |
Null Geodesic Congruences, Asymptotically-Flat Spacetimes and Their Physical Interpretation Adamo, Timothy M. SHEAR FREE CONGRUENCES CENTER OF MASS ANGULAR MOMENTUM |
| title_short |
Null Geodesic Congruences, Asymptotically-Flat Spacetimes and Their Physical Interpretation |
| title_full |
Null Geodesic Congruences, Asymptotically-Flat Spacetimes and Their Physical Interpretation |
| title_fullStr |
Null Geodesic Congruences, Asymptotically-Flat Spacetimes and Their Physical Interpretation |
| title_full_unstemmed |
Null Geodesic Congruences, Asymptotically-Flat Spacetimes and Their Physical Interpretation |
| title_sort |
Null Geodesic Congruences, Asymptotically-Flat Spacetimes and Their Physical Interpretation |
| dc.creator.none.fl_str_mv |
Adamo, Timothy M. Newman, Ezra T. Kozameh, Carlos Nicolas |
| author |
Adamo, Timothy M. |
| author_facet |
Adamo, Timothy M. Newman, Ezra T. Kozameh, Carlos Nicolas |
| author_role |
author |
| author2 |
Newman, Ezra T. Kozameh, Carlos Nicolas |
| author2_role |
author author |
| dc.subject.none.fl_str_mv |
SHEAR FREE CONGRUENCES CENTER OF MASS ANGULAR MOMENTUM |
| topic |
SHEAR FREE CONGRUENCES CENTER OF MASS ANGULAR MOMENTUM |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
A priori, there is nothing very special about shear-free or asymptotically shear-free null geodesic congruences. Surprisingly, however, they turn out to possess a large number of fascinating geometric properties and to be closely related, in the context of general relativity, to a variety of physically significant effects. It is the purpose of this paper to try to fully develop these issues. This work starts with a detailed exposition of the theory of shear-free and asymptotically shear-free null geodesic congruences, i.e., congruences with shear that vanishes at future conformal null infinity. A major portion of the exposition lies in the analysis of the space of regular shear-free and asymptotically shear-free null geodesic congruences. This analysis leads to the space of complex analytic curves in an auxiliary four-complex dimensional space, ℋ-space. They in turn play a dominant role in the applications. The applications center around the problem of extracting interior physical properties of an asymptotically-flat spacetime directly from the asymptotic gravitational (and Maxwell) field itself, in analogy with the determination of total charge by an integral over the Maxwell field at infinity or the identification of the interior mass (and its loss) by (Bondi’s) integrals of the Weyl tensor, also at infinity. More specifically, we will see that the asymptotically shear-free congruences lead us to an asymptotic definition of the center-of-mass and its equations of motion. This includes a kinematic meaning, in terms of the center-of-mass motion, for the Bondi three-momentum. In addition, we obtain insights into intrinsic spin and, in general, angular momentum, including an angular-momentum–conservation law with well-defined flux terms. When a Maxwell field is present, the asymptotically shear-free congruences allow us to determine/define at infinity a center-of-charge world line and intrinsic magnetic dipole moment. Fil: Adamo, Timothy M.. University of Oxford; Reino Unido Fil: Newman, Ezra T.. University of Pittsburgh; Estados Unidos Fil: Kozameh, Carlos Nicolas. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Física Enrique Gaviola. Universidad Nacional de Córdoba. Instituto de Física Enrique Gaviola; Argentina |
| description |
A priori, there is nothing very special about shear-free or asymptotically shear-free null geodesic congruences. Surprisingly, however, they turn out to possess a large number of fascinating geometric properties and to be closely related, in the context of general relativity, to a variety of physically significant effects. It is the purpose of this paper to try to fully develop these issues. This work starts with a detailed exposition of the theory of shear-free and asymptotically shear-free null geodesic congruences, i.e., congruences with shear that vanishes at future conformal null infinity. A major portion of the exposition lies in the analysis of the space of regular shear-free and asymptotically shear-free null geodesic congruences. This analysis leads to the space of complex analytic curves in an auxiliary four-complex dimensional space, ℋ-space. They in turn play a dominant role in the applications. The applications center around the problem of extracting interior physical properties of an asymptotically-flat spacetime directly from the asymptotic gravitational (and Maxwell) field itself, in analogy with the determination of total charge by an integral over the Maxwell field at infinity or the identification of the interior mass (and its loss) by (Bondi’s) integrals of the Weyl tensor, also at infinity. More specifically, we will see that the asymptotically shear-free congruences lead us to an asymptotic definition of the center-of-mass and its equations of motion. This includes a kinematic meaning, in terms of the center-of-mass motion, for the Bondi three-momentum. In addition, we obtain insights into intrinsic spin and, in general, angular momentum, including an angular-momentum–conservation law with well-defined flux terms. When a Maxwell field is present, the asymptotically shear-free congruences allow us to determine/define at infinity a center-of-charge world line and intrinsic magnetic dipole moment. |
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2012 |
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2012-01 |
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article |
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http://hdl.handle.net/11336/268630 Adamo, Timothy M.; Newman, Ezra T.; Kozameh, Carlos Nicolas; Null Geodesic Congruences, Asymptotically-Flat Spacetimes and Their Physical Interpretation; Springer; Living Reviews in Relativity; 15; 1; 1-2012; 1-92 1433-8351 CONICET Digital CONICET |
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http://hdl.handle.net/11336/268630 |
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Adamo, Timothy M.; Newman, Ezra T.; Kozameh, Carlos Nicolas; Null Geodesic Congruences, Asymptotically-Flat Spacetimes and Their Physical Interpretation; Springer; Living Reviews in Relativity; 15; 1; 1-2012; 1-92 1433-8351 CONICET Digital CONICET |
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