antisymmetric tensor;
Einstein gravity;
black hole;
cosmic censorship;
D O I:
10.1016/0370-2693(95)01552-3
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
Classical solutions of the self-interacting, non-abelian antisymmetric tensor gauge theory of Freedman and Townsend coupled to Einstein gravity are discussed. Particularly, it is demonstrated that the theory admits a classical metric solution which, depending on the value of the gauge coupling parameter of the theory, exhibits a black hole with an exotic non-abelian hair or a spacetime showing the ''violation of the cosmic censorship hypothesis'' which should be distinguished from white holes.