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

dc.creatorTorres, Diego F.
dc.creatorRomero, Gustavo Esteban
dc.creatorAnchordoqui, Luis Alfredo
dc.date1998-11-12
dc.date2021-08-13T19:17:59Z
dc.date.accessioned2023-07-15T02:41:29Z
dc.date.available2023-07-15T02:41:29Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/122697
dc.identifierissn:0556-2821
dc.identifierissn:1089-4918
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7462910
dc.descriptionThe 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.
dc.descriptionFacultad de Ciencias Exactas
dc.formatapplication/pdf
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by/4.0/
dc.rightsCreative Commons Attribution 4.0 International (CC BY 4.0)
dc.subjectCiencias Exactas
dc.subjectFísica
dc.subjectPhysics
dc.subjectGravitational microlensing
dc.subjectAstronomy
dc.subjectGamma-ray burst
dc.subjectSignature (topology)
dc.subjectWormhole
dc.subjectSatellite data
dc.subjectObservable
dc.subjectActive galactic nucleus
dc.subjectAstrophysics
dc.subjectNegative mass
dc.titleMight some Gamma Ray Bursts be an observable signature of natural wormholes
dc.typeArticulo
dc.typeArticulo


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