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- W141004873 abstract "The key result of the standard galaxy formation theory is the expectation of a growth of the linear adiabatic perturbations proportional to (1 + Z) −1 (Z is the redshift). It is shown that this expectation need not be correct on small scales; alternatively, a (1 + Z) −2.2 growth is found. From this fact it follows that a categorical rejection of the simplest theory of the galaxy formation - i.e. the theory based on adiabatic perturbations in a baryon dominated universe - is premature" @default.
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- W141004873 date "1993-10-01" @default.
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- W141004873 title "A possible fast growth of adiabatic cosmological perturbations" @default.
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