General Relativistic magneto-hydrodynamical simulations of accretion flows through traversable wormholes
- Autores
- Combi, Luciano; Yang, Huan; Gutiérrez, Eduardo Mario; Noble, Scott C.; Romero, Gustavo Esteban; Campanelli, Manuela
- Año de publicación
- 2024
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present the first dynamical model of plasma accretion onto traversable wormholes by performing General Relativistic magneto-hydrodynamical (GRMHD) simulations of the flow on both sidesof the wormhole. We evolve the ideal MHD equations on a wormhole spacetime described by thespherically symmetric Simpson–Visser metric. The disk is initialized on one side of the wormholeand accretes onto the throat driven by the magneto-rotational instability (MRI). We show that theinflowing plasma quickly settles in the throat and forms a hot, rotating cloud. The wormhole cloudacts as an engine in which gas coming from one side accumulates at the center, dissipates energy, andpowers a mildly relativistic thermal wind toward the other side. Our novel predictions show thataccreting wormholes behave very differently from black holes (BHs) in astrophysical environments.In particular, one mouth presents outflows without accretion signatures, contradicting the jet-disksymbiotic relation that holds for black holes.
Fil: Combi, Luciano. University of Guelph; Canadá. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Yang, Huan. University of Guelph; Canadá
Fil: Gutiérrez, Eduardo Mario. State University Of Pennsylvania. Dept.of Physics; Estados Unidos. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Noble, Scott C.. NASA Goddard Space Flight Center; Estados Unidos
Fil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Campanelli, Manuela. Rochester Institute of Technology; Estados Unidos - Materia
-
General Relativistic magneto-hydrodynamica
Wormholes - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/239222
Ver los metadatos del registro completo
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General Relativistic magneto-hydrodynamical simulations of accretion flows through traversable wormholesCombi, LucianoYang, HuanGutiérrez, Eduardo MarioNoble, Scott C.Romero, Gustavo EstebanCampanelli, ManuelaGeneral Relativistic magneto-hydrodynamicaWormholeshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present the first dynamical model of plasma accretion onto traversable wormholes by performing General Relativistic magneto-hydrodynamical (GRMHD) simulations of the flow on both sidesof the wormhole. We evolve the ideal MHD equations on a wormhole spacetime described by thespherically symmetric Simpson–Visser metric. The disk is initialized on one side of the wormholeand accretes onto the throat driven by the magneto-rotational instability (MRI). We show that theinflowing plasma quickly settles in the throat and forms a hot, rotating cloud. The wormhole cloudacts as an engine in which gas coming from one side accumulates at the center, dissipates energy, andpowers a mildly relativistic thermal wind toward the other side. Our novel predictions show thataccreting wormholes behave very differently from black holes (BHs) in astrophysical environments.In particular, one mouth presents outflows without accretion signatures, contradicting the jet-disksymbiotic relation that holds for black holes.Fil: Combi, Luciano. University of Guelph; Canadá. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: Yang, Huan. University of Guelph; CanadáFil: Gutiérrez, Eduardo Mario. State University Of Pennsylvania. Dept.of Physics; Estados Unidos. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: Noble, Scott C.. NASA Goddard Space Flight Center; Estados UnidosFil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: Campanelli, Manuela. Rochester Institute of Technology; Estados UnidosAmerican Physical Society2024-05info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/239222Combi, Luciano; Yang, Huan; Gutiérrez, Eduardo Mario; Noble, Scott C.; Romero, Gustavo Esteban; et al.; General Relativistic magneto-hydrodynamical simulations of accretion flows through traversable wormholes; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 109; A157; 5-2024; 1-101550-7998CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/prd/abstract/10.1103/PhysRevD.109.103034info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.109.103034info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:38:52Zoai:ri.conicet.gov.ar:11336/239222instacron: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:34982025-09-29 09:38:53.003CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
General Relativistic magneto-hydrodynamical simulations of accretion flows through traversable wormholes |
title |
General Relativistic magneto-hydrodynamical simulations of accretion flows through traversable wormholes |
spellingShingle |
General Relativistic magneto-hydrodynamical simulations of accretion flows through traversable wormholes Combi, Luciano General Relativistic magneto-hydrodynamica Wormholes |
title_short |
General Relativistic magneto-hydrodynamical simulations of accretion flows through traversable wormholes |
title_full |
General Relativistic magneto-hydrodynamical simulations of accretion flows through traversable wormholes |
title_fullStr |
General Relativistic magneto-hydrodynamical simulations of accretion flows through traversable wormholes |
title_full_unstemmed |
General Relativistic magneto-hydrodynamical simulations of accretion flows through traversable wormholes |
title_sort |
General Relativistic magneto-hydrodynamical simulations of accretion flows through traversable wormholes |
dc.creator.none.fl_str_mv |
Combi, Luciano Yang, Huan Gutiérrez, Eduardo Mario Noble, Scott C. Romero, Gustavo Esteban Campanelli, Manuela |
author |
Combi, Luciano |
author_facet |
Combi, Luciano Yang, Huan Gutiérrez, Eduardo Mario Noble, Scott C. Romero, Gustavo Esteban Campanelli, Manuela |
author_role |
author |
author2 |
Yang, Huan Gutiérrez, Eduardo Mario Noble, Scott C. Romero, Gustavo Esteban Campanelli, Manuela |
author2_role |
author author author author author |
dc.subject.none.fl_str_mv |
General Relativistic magneto-hydrodynamica Wormholes |
topic |
General Relativistic magneto-hydrodynamica Wormholes |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
We present the first dynamical model of plasma accretion onto traversable wormholes by performing General Relativistic magneto-hydrodynamical (GRMHD) simulations of the flow on both sidesof the wormhole. We evolve the ideal MHD equations on a wormhole spacetime described by thespherically symmetric Simpson–Visser metric. The disk is initialized on one side of the wormholeand accretes onto the throat driven by the magneto-rotational instability (MRI). We show that theinflowing plasma quickly settles in the throat and forms a hot, rotating cloud. The wormhole cloudacts as an engine in which gas coming from one side accumulates at the center, dissipates energy, andpowers a mildly relativistic thermal wind toward the other side. Our novel predictions show thataccreting wormholes behave very differently from black holes (BHs) in astrophysical environments.In particular, one mouth presents outflows without accretion signatures, contradicting the jet-disksymbiotic relation that holds for black holes. Fil: Combi, Luciano. University of Guelph; Canadá. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina Fil: Yang, Huan. University of Guelph; Canadá Fil: Gutiérrez, Eduardo Mario. State University Of Pennsylvania. Dept.of Physics; Estados Unidos. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina Fil: Noble, Scott C.. NASA Goddard Space Flight Center; Estados Unidos Fil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina Fil: Campanelli, Manuela. Rochester Institute of Technology; Estados Unidos |
description |
We present the first dynamical model of plasma accretion onto traversable wormholes by performing General Relativistic magneto-hydrodynamical (GRMHD) simulations of the flow on both sidesof the wormhole. We evolve the ideal MHD equations on a wormhole spacetime described by thespherically symmetric Simpson–Visser metric. The disk is initialized on one side of the wormholeand accretes onto the throat driven by the magneto-rotational instability (MRI). We show that theinflowing plasma quickly settles in the throat and forms a hot, rotating cloud. The wormhole cloudacts as an engine in which gas coming from one side accumulates at the center, dissipates energy, andpowers a mildly relativistic thermal wind toward the other side. Our novel predictions show thataccreting wormholes behave very differently from black holes (BHs) in astrophysical environments.In particular, one mouth presents outflows without accretion signatures, contradicting the jet-disksymbiotic relation that holds for black holes. |
publishDate |
2024 |
dc.date.none.fl_str_mv |
2024-05 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/239222 Combi, Luciano; Yang, Huan; Gutiérrez, Eduardo Mario; Noble, Scott C.; Romero, Gustavo Esteban; et al.; General Relativistic magneto-hydrodynamical simulations of accretion flows through traversable wormholes; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 109; A157; 5-2024; 1-10 1550-7998 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/239222 |
identifier_str_mv |
Combi, Luciano; Yang, Huan; Gutiérrez, Eduardo Mario; Noble, Scott C.; Romero, Gustavo Esteban; et al.; General Relativistic magneto-hydrodynamical simulations of accretion flows through traversable wormholes; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 109; A157; 5-2024; 1-10 1550-7998 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/prd/abstract/10.1103/PhysRevD.109.103034 info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.109.103034 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
American Physical Society |
publisher.none.fl_str_mv |
American Physical Society |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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1844613229112721408 |
score |
13.070432 |