Initial conditions for supersymmetric inflation

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 56, Issue 8, 1997, Pages 4562-4567

  Lazarides, G ^a   Vlachos, N D ^a  

^a ARISTOTLE UNIVERSITY OF THESSALONIKI   (Greece)

Author keywords

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Indexed keywords

EID: 0000343899     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.56.4562     Document Type: Article

References (9)

1. A. D. Linde, Phys. Rev. D 49, 748 (1994).
2. G. Lazarides and C. Panagiotakopoulos, Phys. Rev. D 52, R559 (1995).
3. G. Dvali, Q. Shafi, and R. Schaefer, Phys. Rev. Lett. 73, 1886 (1994).
4. G. Lazarides, R. K. Schaefer, and Q. Shafi, Phys. Rev. D 56, 1324 (1997).
5. G. Lazarides, C. Panagiotakopoulos, and N. D. Vlachos, Phys. Rev. D 54, 1369 (1996).
6. For an earlier attempt at inflation with this superpotential, see E. J. Copeland, A. R. Liddle, D. H. Lyth, E. D. Stewart, and D. Wands, Phys. Rev. D 49, 6410 (1994).
7. Supersymmetric inflation has a long history and there are several reviews available, see, e.g., A. D. Linde, Particle Physics and Inflationary Cosmology (Harwood Academic, Switzerland, 1990).
8. M. Turner, Phys. Rev. D 28, 1243 (1983).
9. W. H. Press, S. A. Teukolsky, W. T. Vetterling, and B. P. Flannery, Numerical Recipes in Fortran: The Art of Scientific Computing, 2nd ed. (Cambridge University Press, Cambridge, England, 1992).