摘要

Axially symmetric Bianchi type-I space time is considered in the presence of massless scalar field and cosmic strings in Barber's (Gen. Relativ. Gravit. 14:117, 1982) self-creation theory with two conditions (i) A=B (n) and (ii) epsilon+lambda=0. Some physical and kinematical properties of the model, thus obtained, are also discussed.

  • 出版日期2010-5