Astronomy and Astrophysics – Astrophysics
Scientific paper
1999-07-07
Phys.Rev. D60 (1999) 103512
Astronomy and Astrophysics
Astrophysics
4 pages, no figure, To appear in Phys. Rev. D
Scientific paper
10.1103/PhysRevD.60.103512
We introduce a scalar-type perturbation variable $\Phi$ which is conserved in
the large-scale limit considering general sign of three-space curvature ($K$),
the cosmological constant ($\Lambda$), and time varying equation of state. In a
pressureless medium $\Phi$ is {\it exactly conserved} in all scales.
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