dc.creatorGallo, Emanuel
dc.creatorMoreschi, Osvaldo Mario
dc.date.accessioned2021-02-01T18:19:43Z
dc.date.accessioned2022-10-15T16:03:09Z
dc.date.available2021-02-01T18:19:43Z
dc.date.available2022-10-15T16:03:09Z
dc.date.created2021-02-01T18:19:43Z
dc.date.issued2019-09
dc.identifierGallo, Emanuel; Moreschi, Osvaldo Mario; Modeling the dynamics of black holes through balanced equations of motion in the null gauge; World Scientific; International Journal of Geometric Methods in Modern Physics; 16; 9; 9-2019; 1-39; 1950131
dc.identifier0219-8878
dc.identifierhttp://hdl.handle.net/11336/124405
dc.identifier1793-6977
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4406533
dc.description.abstractWe develop further the general framework for modeling the dynamics of the motion of black holes, presented in [E. Gallo and O. M. Moreschi, Modeling the dynamics of black holes through balanced equations of motion, Int. J. Geom. Meth. Mod. Phys. 16(3) (2019) 1950034], by employing a convenient null gauge, in general relativity, for the construction of the balanced equations of motion. This null gauge has the property that the asymptotic structure is intimately related to the interior one; in particular there is a strong connection between the field equations and the balanced equations of motion. Our work is very related to what we have called "Robinson-Trautman (RT) geometries" [S. Dain, O. M. Moreschi and R. J. Gleiser, Photon rockets and the Robinson-Trautman geometries, Class. Quantum Grav. 13(5) (1996) 1155-1160] in the past. These geometries are used in the sense of the general framework, we have presented in [E. Gallo and O. M. Moreschi, Modeling the dynamics of black holes through balanced equations of motion, Int. J. Geom. Meth. Mod. Phys. 16(3) (2019) 1950034]. We present the balanced equations of motion in second order of the acceleration. We solve the required components of the field equation at their respective required orders, G2 and G3, in terms of the gravitational constant. We indicate how this approach can be extended to higher orders.
dc.languageeng
dc.publisherWorld Scientific
dc.relationinfo:eu-repo/semantics/altIdentifier/url/https://www.worldscientific.com/doi/10.1142/S0219887819501317
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/https://doi.org/10.1142/S0219887819501317
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/restrictedAccess
dc.subjectBLACK HOLES
dc.subjectEQUATION OF MOTION
dc.subjectGRAVITATIONAL RADIATION
dc.titleModeling the dynamics of black holes through balanced equations of motion in the null gauge
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:ar-repo/semantics/artículo
dc.typeinfo:eu-repo/semantics/publishedVersion


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