On Uniqueness of Kerr Space-time near null infinity

Simple item page
dc.creatorWu, Xiaoning
dc.creatorBai, Shan
dc.date2008-11-24
dc.date.accessioned2026-07-07T12:22:37Z
dc.date.available2026-07-07T12:22:37Z
dc.descriptionWe re-express the Kerr metric in standard Bondi-Saches' coordinate near null infinity ${\cal I}^+$. Using the uniqueness result of characteristic initial value problem, we prove the Kerr metric is the only asymptotic flat, stationary, axial symmetric, Type-D solution of vacuum Einstein equation. The Taylor series of Kerr space-time is expressed in terms of B-S coordinates and the N-P constants have been calculated.
dc.description15pages
dc.identifierhttps://arxiv.org/abs/0811.3794
dc.identifierhttp://arxiv.org/abs/0811.3794
dc.identifierPhys.Rev.D78:124009,2008
dc.identifierdoi:10.1103/PhysRevD.78.124009
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/213714
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleOn Uniqueness of Kerr Space-time near null infinity
dc.typetext

Files

Collections

arXiv