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Steinhardt has also suggested parametrizing the equation of state of the smooth component; see, P. J. Steinhardt, in Critical Dialogues in Cosmology, edited by N. Turok (World Scientific, Singapore, 1997)
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Steinhardt has also suggested parametrizing the equation of state of the smooth component; see, P. J. Steinhardt, in Critical Dialogues in Cosmology, edited by N. Turok (World Scientific, Singapore, 1997).
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45
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85038296072
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The second problem could be circumvented by having the smooth component come into existence recently, e.g., a relativistic sea of particles (Formula presented) can be created by the decay of unstable CDM (see Ref. 12
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The second problem could be circumvented by having the smooth component come into existence recently, e.g., a relativistic sea of particles (Formula presented) can be created by the decay of unstable CDM (see Ref. 12).
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The Taylor series expansion is not very accurate, even for (Formula presented) Padé approximants provide a more accurate approximation, e.g., the second-order Padé approximant is (Formula presented) For all of our results we have numerically integrated the expression for (Formula presented)
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The Taylor series expansion is not very accurate, even for (Formula presented) Padé approximants provide a more accurate approximation, e.g., the second-order Padé approximant is (Formula presented) For all of our results we have numerically integrated the expression for (Formula presented)
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