Might some Gamma Ray Bursts be an observable signature of natural wormholes

Autores
Torres, Diego F.; Romero, Gustavo Esteban; Anchordoqui, Luis Alfredo
Año de publicación
1998
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The extragalactic microlensing scenario for natural wormholes is examined. It is shown that the main features of wormhole lensing events upon the light of distant active galactic nuclei are similar to some types of already observed gamma ray bursts (GRBs). Using recent satellite data on GRBs, an upper limit to the negative mass density, O(10−36)g cm−3 under the form of wormholelike objects is presented.
Facultad de Ciencias Exactas
Materia
Ciencias Exactas
Física
Physics
Gravitational microlensing
Astronomy
Gamma-ray burst
Signature (topology)
Wormhole
Satellite data
Observable
Active galactic nucleus
Astrophysics
Negative mass
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/122697
Acceder
id SEDICI_378959197fb28eb9b7dee6d983d5e3a3
oai_identifier_str oai:sedici.unlp.edu.ar:10915/122697
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling Might some Gamma Ray Bursts be an observable signature of natural wormholesTorres, Diego F.Romero, Gustavo EstebanAnchordoqui, Luis AlfredoCiencias ExactasFísicaPhysicsGravitational microlensingAstronomyGamma-ray burstSignature (topology)WormholeSatellite dataObservableActive galactic nucleusAstrophysicsNegative massThe extragalactic microlensing scenario for natural wormholes is examined. It is shown that the main features of wormhole lensing events upon the light of distant active galactic nuclei are similar to some types of already observed gamma ray bursts (GRBs). Using recent satellite data on GRBs, an upper limit to the negative mass density, O(10<sup>−36</sup>)g cm<sup>−3</sup> under the form of wormholelike objects is presented.Facultad de Ciencias Exactas1998-11-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/122697enginfo:eu-repo/semantics/altIdentifier/issn/0556-2821info:eu-repo/semantics/altIdentifier/issn/1089-4918info:eu-repo/semantics/altIdentifier/arxiv/astro-ph/9802106info:eu-repo/semantics/altIdentifier/doi/10.1103/physrevd.58.123001info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/4.0/Creative Commons Attribution 4.0 International (CC BY 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-22T17:10:09Zoai:sedici.unlp.edu.ar:10915/122697Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 17:10:09.424SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Might some Gamma Ray Bursts be an observable signature of natural wormholes
title Might some Gamma Ray Bursts be an observable signature of natural wormholes
spellingShingle Might some Gamma Ray Bursts be an observable signature of natural wormholes
Torres, Diego F.
Ciencias Exactas
Física
Physics
Gravitational microlensing
Astronomy
Gamma-ray burst
Signature (topology)
Wormhole
Satellite data
Observable
Active galactic nucleus
Astrophysics
Negative mass
title_short Might some Gamma Ray Bursts be an observable signature of natural wormholes
title_full Might some Gamma Ray Bursts be an observable signature of natural wormholes
title_fullStr Might some Gamma Ray Bursts be an observable signature of natural wormholes
title_full_unstemmed Might some Gamma Ray Bursts be an observable signature of natural wormholes
title_sort Might some Gamma Ray Bursts be an observable signature of natural wormholes
dc.creator.none.fl_str_mv Torres, Diego F.
Romero, Gustavo Esteban
Anchordoqui, Luis Alfredo
author Torres, Diego F.
author_facet Torres, Diego F.
Romero, Gustavo Esteban
Anchordoqui, Luis Alfredo
author_role author
author2 Romero, Gustavo Esteban
Anchordoqui, Luis Alfredo
author2_role author
author
dc.subject.none.fl_str_mv Ciencias Exactas
Física
Physics
Gravitational microlensing
Astronomy
Gamma-ray burst
Signature (topology)
Wormhole
Satellite data
Observable
Active galactic nucleus
Astrophysics
Negative mass
topic Ciencias Exactas
Física
Physics
Gravitational microlensing
Astronomy
Gamma-ray burst
Signature (topology)
Wormhole
Satellite data
Observable
Active galactic nucleus
Astrophysics
Negative mass
dc.description.none.fl_txt_mv The extragalactic microlensing scenario for natural wormholes is examined. It is shown that the main features of wormhole lensing events upon the light of distant active galactic nuclei are similar to some types of already observed gamma ray bursts (GRBs). Using recent satellite data on GRBs, an upper limit to the negative mass density, O(10<sup>−36</sup>)g cm<sup>−3</sup> under the form of wormholelike objects is presented.
Facultad de Ciencias Exactas
description The extragalactic microlensing scenario for natural wormholes is examined. It is shown that the main features of wormhole lensing events upon the light of distant active galactic nuclei are similar to some types of already observed gamma ray bursts (GRBs). Using recent satellite data on GRBs, an upper limit to the negative mass density, O(10<sup>−36</sup>)g cm<sup>−3</sup> under the form of wormholelike objects is presented.
publishDate 1998
dc.date.none.fl_str_mv 1998-11-12
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Articulo
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://sedici.unlp.edu.ar/handle/10915/122697
url http://sedici.unlp.edu.ar/handle/10915/122697
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/0556-2821
info:eu-repo/semantics/altIdentifier/issn/1089-4918
info:eu-repo/semantics/altIdentifier/arxiv/astro-ph/9802106
info:eu-repo/semantics/altIdentifier/doi/10.1103/physrevd.58.123001
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by/4.0/
Creative Commons Attribution 4.0 International (CC BY 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by/4.0/
Creative Commons Attribution 4.0 International (CC BY 4.0)
dc.format.none.fl_str_mv application/pdf
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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score 12.982451

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