Bel-Robinson tensor;
factorizations;
principal null directions;
gravitational energy;
D O I:
10.1023/A:1018844727612
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
Recently Bonilla and Senovilla studied factorizations of the symmetric and tracefree rank four Bel-Robinson tensor T-abcd into two symmetric tracefree rank two tensors. While the Bel-Robinson tensor has the dimension of energy density squared, each of these factors has the dimension of energy density. When the two factors can be chosen to be equal they are called the "square root" of T-abcd The approach used was purely tensorial. In this paper we use spinors and show that the factors can be found in a very simple way using the principal null directions of the Weyl tenser. We obtain a factorization of the Weyl spinor into two symmetric rank two spinors, which when multiplied by their complex conjugates give the tracefree and symmetric factors of T-abcd. The factorization is immediately seen to be non-unique in most cases and the number of essentially non-equivalent factorizations becomes clear. It also becomes obvious that the square root only can exist in spacetimes of Petrov types N, D and O, in which cases one can equally well speak about the "square root" of the Weyl spinor. Explicit formulas for the factors of the Weyl spinor are given for all Petrov types.