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dc.date.accessioned 2020-08-11T17:09:11Z
dc.date.available 2020-08-11T17:09:11Z
dc.date.issued 2017-10
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/101952
dc.description.abstract We analyze the energy configuration of a charged black hole in the TeleparallelFramework of General Relativity. We obtain the energy-momentum tensor of the gravitationalfield in a stationary frame, and we calculate its contribution to the total energyof the system. We study the same gravitational field measured by an accelerated frameand we analyze how the energy-momentum tensor is transformed. We found that in theaccelerated frame, a Poyinting-like flux appears for the gravitational field but not for theelectromagnetic field. en
dc.language en es
dc.subject Gravitational fields es
dc.subject General relativity es
dc.subject Blacks holes es
dc.title Gravitational energy and radiation of a charged black hole en
dc.type Articulo es
sedici.identifier.uri https://ri.conicet.gov.ar/11336/35353 es
sedici.identifier.uri http://stacks.iop.org/0264-9381/34/i=19/a=195008?key=crossref.3174d5c368db8d92efb5d5ddbc236d73 es
sedici.identifier.other http://doi.org/10.1088/1361-6382/aa86c9 es
sedici.identifier.other hdl:11336/35353 es
sedici.identifier.issn 0264-9381 es
sedici.creator.person Combi, Luciano es
sedici.creator.person Romero, Gustavo Esteban es
sedici.subject.materias Ciencias Astronómicas es
sedici.subject.materias Física es
sedici.description.fulltext true es
mods.originInfo.place Instituto Argentino de Radioastronomía es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Preprint es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Classical and Quantum Gravity es
sedici.relation.journalVolumeAndIssue vol. 34, no. 19 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)