메뉴 건너뛰기




Volumn 55, Issue 4, 2001, Pages 458-464

Influence of the cosmological expansion on small systems

Author keywords

[No Author keywords available]

Indexed keywords


EID: 0035797337     PISSN: 02955075     EISSN: None     Source Type: Journal    
DOI: 10.1209/epl/i2001-00437-y     Document Type: Article
Times cited : (18)

References (18)
  • 8
    • 0003817141 scopus 로고
    • John Wiley & Sons
    • WEINBERG S., Gravitation & Cosmology (John Wiley & Sons) 1972; PEEBLES P. J. E., Principles of Physical Cosmology (Princenton University Press) 1993; PADMANABHAN T., Structure Formation in the Universe (Cambridge University Press) 1993.
    • (1972) Gravitation & Cosmology
    • Weinberg, S.1
  • 9
    • 0004014244 scopus 로고
    • Princenton University Press
    • WEINBERG S., Gravitation & Cosmology (John Wiley & Sons) 1972; PEEBLES P. J. E., Principles of Physical Cosmology (Princenton University Press) 1993; PADMANABHAN T., Structure Formation in the Universe (Cambridge University Press) 1993.
    • (1993) Principles of Physical Cosmology
    • Peebles, P.J.E.1
  • 10
    • 0003635793 scopus 로고
    • Cambridge University Press
    • WEINBERG S., Gravitation & Cosmology (John Wiley & Sons) 1972; PEEBLES P. J. E., Principles of Physical Cosmology (Princenton University Press) 1993; PADMANABHAN T., Structure Formation in the Universe (Cambridge University Press) 1993.
    • (1993) Structure Formation in the Universe
    • Padmanabhan, T.1
  • 12
    • 0007221921 scopus 로고    scopus 로고
    • ij(0) is computed for the RW picture (see right before eq. (8)), eq. (1) then becomes the Newtonian limit of the equation for geodesic deviation in Fermi normal coordinates, as computed in ref. [5]
    • ij(0) is computed for the RW picture (see right before eq. (8)), eq. (1) then becomes the Newtonian limit of the equation for geodesic deviation in Fermi normal coordinates, as computed in ref. [5].
  • 15
    • 0007237875 scopus 로고    scopus 로고
    • The presence of a cosmological constant would contribute in eq. (5). But, for a time-independent cosmological constant, this contribution is just a static effect and does not affect the effective Hubble constant, eq. (7)
    • The presence of a cosmological constant would contribute in eq. (5). But, for a time-independent cosmological constant, this contribution is just a static effect and does not affect the effective Hubble constant, eq. (7).
  • 17
    • 0007229707 scopus 로고    scopus 로고
    • 3) is very large
    • 3) is very large.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.