메뉴 건너뛰기




Volumn 381, Issue 4, 1996, Pages 413-419

The spectrum of cosmological perturbations produced by a multi-component inflaton to second order in the slow-roll approximation

Author keywords

Cosmology; Inflation; Perturbations

Indexed keywords


EID: 0001401477     PISSN: 03702693     EISSN: None     Source Type: Journal    
DOI: 10.1016/0370-2693(96)00594-1     Document Type: Article
Times cited : (102)

References (9)
  • 1
    • 0003753693 scopus 로고
    • Harwood Academic, Switzerland
    • A.D. Linde, Particle physics and inflationary cosmology (Harwood Academic, Switzerland, 1990); E.W. Kolb and M.S. Turner, The early universe (Addison-Wesley, New York, 1990).
    • (1990) Particle Physics and Inflationary Cosmology
    • Linde, A.D.1
  • 2
    • 0004210614 scopus 로고
    • Addison-Wesley, New York
    • A.D. Linde, Particle physics and inflationary cosmology (Harwood Academic, Switzerland, 1990); E.W. Kolb and M.S. Turner, The early universe (Addison-Wesley, New York, 1990).
    • (1990) The Early Universe
    • Kolb, E.W.1    Turner, M.S.2
  • 3
    • 34748923788 scopus 로고
    • A.H. Guth and S.-Y. Pi, Phys. Rev. Lett. 49 (1982) 1110; J.M. Bardeen, P.J. Steinhardt and M.S. Turner, Phys. Rev. D 28 (1983) 679; A.R. Liddle and D.H. Lyth, Phys. Lett. B 291 (1992) 391.
    • (1982) Phys. Rev. Lett. , vol.49 , pp. 1110
    • Guth, A.H.1    Pi, S.-Y.2
  • 4
    • 33744767932 scopus 로고
    • A.H. Guth and S.-Y. Pi, Phys. Rev. Lett. 49 (1982) 1110; J.M. Bardeen, P.J. Steinhardt and M.S. Turner, Phys. Rev. D 28 (1983) 679; A.R. Liddle and D.H. Lyth, Phys. Lett. B 291 (1992) 391.
    • (1983) Phys. Rev. D , vol.28 , pp. 679
    • Bardeen, J.M.1    Steinhardt, P.J.2    Turner, M.S.3
  • 5
    • 0004303445 scopus 로고
    • A.H. Guth and S.-Y. Pi, Phys. Rev. Lett. 49 (1982) 1110; J.M. Bardeen, P.J. Steinhardt and M.S. Turner, Phys. Rev. D 28 (1983) 679; A.R. Liddle and D.H. Lyth, Phys. Lett. B 291 (1992) 391.
    • (1992) Phys. Lett. B , vol.291 , pp. 391
    • Liddle, A.R.1    Lyth, D.H.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.