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Volumn 63, Issue 10, 2001, Pages

Evolution of cosmological models in the brane-world scenario

Author keywords

[No Author keywords available]

Indexed keywords

ANISOTROPY; ARTICLE; COSMOS; DYNAMICS; MODEL; SPACE; TECHNIQUE;

EID: 84890387875     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.63.104012     Document Type: Article
Times cited : (135)

References (54)
  • 8
    • 33744637978 scopus 로고
    • edited by K. Kikkawa, N. Nakanishi, and H. Nariai Springer-Verlag, New York
    • K. Akama, in Lectures in Physics, Vol. 176, edited by K. Kikkawa, N. Nakanishi, and H. Nariai (Springer-Verlag, New York, 1982).
    • (1982) Lectures in Physics , vol.176
    • Akama, K.1
  • 15
    • 17044402199 scopus 로고    scopus 로고
    • 61, 023506 (1999);
    • (1999) Phys. Rev. D , vol.61 , pp. 023506
  • 28
    • 34347209717 scopus 로고    scopus 로고
    • D. J. H. Chung, H. Davoudiasl, and L. Everett, hep-ph/0010103
    • D. J. H. Chung, H. Davoudiasl, and L. Everett, hep-ph/0010103.
  • 35
    • 0004057466 scopus 로고
    • The University of Chicago Press, Chicago
    • R. M. Wald, General Relativity (The University of Chicago Press, Chicago, 1984).
    • (1984) General Relativity
    • Wald, R.M.1
  • 44
  • 47
    • 34347213692 scopus 로고    scopus 로고
    • note
    • The presence of a zero eigenvalue is (excepting in the case of the Einstein Universe critical points) a consequence of having a dynamical system with a constraint: The Friedmann equation. If we had used it to eliminate one variable and reduce the dimension of the state space, we svould not find any vanishing eigenvalue. In conclusion, this fact does not affect the hyperbolic character of the critical points.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.