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Extreme binary black holes in a physical representation
dc.contributor.author | Cabrera Munguia, Ivan | |
dc.date.accessioned | 2018-12-07T17:02:45Z | |
dc.date.available | 2018-12-07T17:02:45Z | |
dc.date.issued | 2018-10-31 | |
dc.identifier.uri | http://cathi.uacj.mx/20.500.11961/4642 | |
dc.description.abstract | Stationary axisymmetric binary systems of unequal co- and counter-rotating extreme Kerr black holes separated by a conical singularity are studied. Both solutions are identified as two three- parametric subfamilies of the Kinnersley–Chitre metric, and fully depicted by Komar parameters: the two masses M1 and M2, and a coordinate distance R, where the angular momenta J1 and J2 are functions of these parameters. Our physical representation allows us to identify clearly some limits and novel physical properties. | es_MX |
dc.description.uri | https://academic.oup.com/ptep/article/2018/10/103E01/5150479 | es_MX |
dc.language.iso | en | es_MX |
dc.relation.ispartof | Producto de investigación IIT | es_MX |
dc.relation.ispartof | Instituto de Ingeniería y Tecnología | es_MX |
dc.rights | Atribución-NoComercial-SinDerivadas 2.5 México | * |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/2.5/mx/ | * |
dc.subject | Extreme sources | es_MX |
dc.subject | binary black holes | es_MX |
dc.subject.other | info:eu-repo/classification/cti/1 | es_MX |
dc.title | Extreme binary black holes in a physical representation | es_MX |
dc.type | Artículo | es_MX |
dcterms.thumbnail | http://ri.uacj.mx/vufind/thumbnails/rupiiit.png | es_MX |
dcrupi.instituto | Instituto de Ingeniería y Tecnología | es_MX |
dcrupi.cosechable | Si | es_MX |
dcrupi.norevista | 2018 | es_MX |
dcrupi.volumen | 103E01 | es_MX |
dcrupi.nopagina | 1-13 | es_MX |
dc.identifier.doi | 10.1093/ptep/pty108 | es_MX |
dc.journal.title | Progress of Theoretical and Experimental Physics | es_MX |
dc.lgac | Sin línea de generación | es_MX |
dc.cuerpoacademico | Sin cuerpo académico | es_MX |