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8
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0003817141
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John Wiley & Sons
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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.
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(1972)
Gravitation & Cosmology
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Weinberg, S.1
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9
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0004014244
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Princenton University Press
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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.
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(1993)
Principles of Physical Cosmology
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Peebles, P.J.E.1
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10
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-
0003635793
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Cambridge University Press
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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.
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(1993)
Structure Formation in the Universe
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Padmanabhan, T.1
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11
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-
14544286907
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edited by ERIGUCHI Y. et al., and references therein; gr-qc/0001056
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BUCHERT T., Proceedings of the 9th JGRG Meeting, Hiroshima 1999, edited by ERIGUCHI Y. et al., 2000, p. 306, and references therein; gr-qc/0001056.
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(2000)
Proceedings of the 9th JGRG Meeting, Hiroshima 1999
, pp. 306
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Buchert, T.1
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12
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-
0007221921
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-
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]
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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].
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-
-
-
15
-
-
0007237875
-
-
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)
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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).
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-
-
-
17
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-
0007229707
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3) is very large
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3) is very large.
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