Cosmic strings;
Viscous fluid;
Bianchi type II models;
VIII;
D O I:
10.1007/s10773-010-0351-0
中图分类号:
O4 [物理学];
学科分类号:
0702 ;
摘要:
Some Bianchi type II bulk viscous string cosmological models with electromagnetic field are investigated. To get a determinate solution, we assume the shear (sigma) is proportional to the expansion (theta), which leads to a supplementary condition B=lA (n) , between metric potentials, is used where A and B are function of time alone. A particular solution for n=0 is also discussed. The physical and geometrical implications of the models are discussed.