Aros R, Contreras M, Olea R, Troncoso R, Zanelli J
Centro de Estudios Cientificos de Santiago, Casilla 16443, Santiago 9, Chile and Universidad Nacional Andres Bello, Sazie 2320, Santiago, Chile.
Phys Rev Lett. 2000 Feb 21;84(8):1647-50. doi: 10.1103/PhysRevLett.84.1647.
A new formula for the conserved charges in 3+1 gravity for spacetimes with local anti-de Sitter asymptotic geometry is proposed. It is shown that requiring the action to have an extremum for this class of asymptotia sets the boundary term that must be added to the Lagrangian as the Euler density with a fixed weight factor. The resulting action gives rise to the mass and angular momentum as Noether charges associated to the asymptotic Killing vectors without requiring specification of a reference background in order to have a convergent expression. A consequence of this definition is that any negative constant curvature spacetime has vanishing Noether charges. These results remain valid in the Lambda = 0 limit.
提出了一种适用于具有局部反德西特渐近几何的时空的3 + 1维引力中守恒电荷的新公式。结果表明,要求该作用量对于此类渐近性具有极值,会确定必须作为具有固定权重因子的欧拉密度添加到拉格朗日量中的边界项。由此产生的作用量产生了作为与渐近克利福德向量相关的诺特定理电荷的质量和角动量,而无需指定参考背景即可得到收敛表达式。此定义的一个结果是,任何负常曲率时空的诺特定理电荷都为零。这些结果在Λ = 0的极限情况下仍然有效。