메뉴 건너뛰기




Volumn 66, Issue 2, 2002, Pages

Gravitational equilibrium in the presence of a positive cosmological constant

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; COSMOS; GEOMETRY; GRAVITY; MATHEMATICAL ANALYSIS; MATHEMATICAL MODEL; STEADY STATE;

EID: 0037101451     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.66.023003     Document Type: Article
Times cited : (32)

References (22)
  • 8
    • 33847404218 scopus 로고    scopus 로고
    • R. Aldrovandi and J.G. Pereira, gr-qc/9809061
    • R. Aldrovandi and J.G. Pereira, gr-qc/9809061;
  • 9
    • 33847416105 scopus 로고    scopus 로고
    • R. Aldrovandi, A.L. Barbosa, L.C.B. Crispino, and J.G. Pereira, gr-qc/9801100
    • R. Aldrovandi, A.L. Barbosa, L.C.B. Crispino, and J.G. Pereira, gr-qc/9801100.
  • 12
    • 33847366011 scopus 로고    scopus 로고
    • L. Bergström and U. Danielsson, astro-ph/0002152
    • L. Bergström and U. Danielsson, astro-ph/0002152.
  • 18
    • 33847341875 scopus 로고    scopus 로고
    • note
    • In making this statement, we have to be careful insofar as the densities for superclusters are often extracted from the virial theorem with Λ = 0. Hence we have to trust that the "true" values of the densities are not very far from the quoted ones. Since for flattened systems as superclusters, A in Eq. (15) will be quite sizeable, it is still true that superclusters are most likely not in gravitational equilibrium unless we are ready to increase the presently known values of their densities by orders of magnitude.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.