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Volumn 50, Issue 2, 1994, Pages 627-631

Small scale integrated Sachs-Wolfe effect

Author keywords

[No Author keywords available]

Indexed keywords


EID: 0000925915     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.50.627     Document Type: Article
Times cited : (56)

References (28)
  • 2
    • 84927337798 scopus 로고    scopus 로고
    • Note that what is here called the ``ordinary'' and ``integrated'' Sachs-Wolfe effects are both contained in the general formulas of this paper.
  • 3
    • 84927337797 scopus 로고    scopus 로고
    • W. Hu and N. Sugiyama (unpublished); W. Hu, in Proceedings of the Case Western CMB Meeting, edited by L. Krauss, (unpublished). We provide a unified treatment comparing and contrasting the physical basis of each effect for isocurvature versus adiabatic initial conditions.
  • 5
    • 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
  • 12
    • 84927337796 scopus 로고    scopus 로고
    • The Vishniac effect dominates over ISW in many models for k η0>wig 105.
  • 20
    • 84927337794 scopus 로고    scopus 로고
    • Gauge choice is, of course, irrelevant for our small-scale calculation.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.