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2004/10/29 | E-de S宇宙模型[Einstein-de Sitter Cosmological Model]
类别(Ω〖物理〗)
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发表于 15:04
A cosmological model (not to be confused with the
de Sitter cosmological model
)which assumes a homogeneous, isotropic, constant curvature
universe
with zero
cosmological constant
and pressure
P
,
(1)
Its equation of motion, derived from the
Einstein field equations
, is
(2)
where
a
is the
expansion parameter
,
H
is the
Hubble constant
,
G
is the
gravitational constant
,and
is the density. For constant mass of the
universe
M
,
(3)
(4)
(5)
(6)
(7)
(8)
Therefore,
(9)
so
(10)
For small densities,
(11)
(12)
(13)
(14)
(15)
0
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