Evolution of cosmological perturbations in a stage dominated by an oscillatory scalar field

Progress of Theoretical Physics

Volumn 96, Issue 5, 1996, Pages 949-970

  Kodama, Hideo ^b   Hamazaki, Takashi ^a  

^a KYOTO UNIVERSITY   (Japan)

^b KYOTO UNIVERSITY   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0030363402     PISSN: 0033068X     EISSN: None     Source Type: Journal    
DOI: 10.1143/PTP.96.949     Document Type: Article

References (13)

1. S. W. Hawking, Phys. Lett. B115 (1982), 295.
2. A. H. Guth and S.-Y. Pi, Phys. Rev. Lett. 49 (1982), 1110.
3. A. A. Starobinsky, Phys. Lett. B117 (1982), 175.
4. J. M. Bardeen, P. J. Steinhardt and M. S. Turner, Phys. Rev. D28 (1983), 679.
5. J. A. Friemann and M. S. Turner, Phys. Rev. D30 (1984), 265.
6. R. Brandenberger and R. Kahn, Phys. Rev. D29 (1984), 2172.
7. H. Kodama and M. Sasaki, Prog. Theor. Phys. Suppl. No. 78 (1984).
8. D. Polarski and A. A. Starobinsky, Nucl. Phys. B385 (1992), 623.
9. V. F. Mukhanov, Sov. Phys.-JETP 68 (1988), 1297.
10. J. M. Bardeen, Phys. Rev. D22 (1980), 1882.
11. N. Makino and M. Sasaki, Prog. Theor. Phys. 86 (1991), 103.
12. Y. Shatanov, J. Traschen and R. Brandenberger, Phys. Rev. D51 (1995), 5438.
13. Y. Nambu and M. Sasaki, Phys. Rev. D42 (1990), 3918.