西南石油大学学报(自然科学版) ›› 1993, Vol. 15 ›› Issue (3): 135-138.DOI: 10.3863/j.issn.1000-2634.1993.03.019

• 物理数学 • Previous Articles     Next Articles

INITIAL CONDITIONS FOR INFLATION IN GENERALIZED EINSTEIN THEO-RIES

wang wen-fu
  

  1. (Dept. of Basie Courses)
  • Received:1992-10-25 Revised:1900-01-01 Online:1993-08-20 Published:1993-08-20
  • Contact: wang wen-fu

Abstract: This paper calculates the cosmic wave function for a cosmological model with two scalar fields:one is the etandard inflation whose potential is exponentially coupled to the other field. If the scale factor a is thought of as a time variable,the initial values of cp and x for the success of inflation are obtained .If the scalar to be quantum mechanically stabilized with a most probable radius of the Planck length.

Key words: Cosmology wheeler-Dcwitt equation Cosmic intlat

CLC Number: