메뉴 건너뛰기




Volumn 51, Issue 6, 1995, Pages 2599-2630

Toward understanding CMB anisotropies and their implications

Author keywords

[No Author keywords available]

Indexed keywords


EID: 33644978258     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.51.2599     Document Type: Article
Times cited : (233)

References (70)
  • 11
    • 0002504178 scopus 로고
    • On the anisotropy of the cosmological background matter and radiation distribution. II - The radiation anisotropy in models with negative spatial curvature
    • (1983) The Astrophysical Journal , vol.273 , pp. 2
    • Wilson, M.L.1
  • 17
    • 84927495785 scopus 로고    scopus 로고
    • Note that his ΦH = Φ and ΦA = Ψ.
  • 24
    • 84927492238 scopus 로고    scopus 로고
    • Their definition of the radial eigenfunctions is equivalent to our Ml1/2 Xνl, see also, Ref. 22
  • 26
    • 84927462115 scopus 로고    scopus 로고
    • The stability problem can be avoided by two tricks: rewrite the Boltzmann equation with Δγ replacing Theta0 and Theta'l = Ml1/2 Thetal instead of Thetal.
  • 43
    • 84927459171 scopus 로고    scopus 로고
    • G. Efstathiou, Large Scale Motions in the Universe: A Vatican Study Week, edited by V. C. Rubin and G. V. Coyne (Princeton University Press, Princeton, 1988), p. 299.
  • 49
    • 84927463550 scopus 로고    scopus 로고
    • Gravitational potential fluctuations per logarithmic k interval are predicted to be constant implying constant anisotropy contributions through Eq. (9) up to the curvature cutoff.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.