Remarks on the Theory of Cosmological Perturbation
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Abstract
It is shown that the power spectrum defined in the Synchronous gauge can not be directly used to calculate the predictions of cosmological models on the large-scale structure of Universe, which should be calculated directly by a suitable gauge-invariant power spectrum or the power spectrum defined in the Newtonian Gauge.
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Cite this article:
LIN Wen-Bin. Remarks on the Theory of Cosmological Perturbation[J]. Chin. Phys. Lett., 2001, 18(11): 1539-1542.
LIN Wen-Bin. Remarks on the Theory of Cosmological Perturbation[J]. Chin. Phys. Lett., 2001, 18(11): 1539-1542.
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LIN Wen-Bin. Remarks on the Theory of Cosmological Perturbation[J]. Chin. Phys. Lett., 2001, 18(11): 1539-1542.
LIN Wen-Bin. Remarks on the Theory of Cosmological Perturbation[J]. Chin. Phys. Lett., 2001, 18(11): 1539-1542.
|