isocurvatureの例文

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While the overall constraints are inconclusive, uncorrelated isocurvature cold dark matter modes are found to be unlikely.
For instance, in 1987, he proposed the primordial isocurvature baryon model for the development of the early universe.
For isocurvature fluctuations, the density variations for one component do not necessarily correspond to density variations in other components.
While it is usually assumed that the initial fluctuations are adiabatic, the possibility of isocurvature fluctuations can be considered given current cosmological data.
Silk damping is not as significant in models of cosmological development which posit early isocurvature fluctuations ( i . e . fluctuations which do not require a constant ratio of baryons and photons ).
Isocurvature density perturbations produce a series of peaks whose angular scales ( " l " values of the peaks ) are roughly in the ratio 1 : 3 : 5 : . . ., while adiabatic density perturbations produce peaks whose locations are in the ratio 1 : 2 : 3 : . . . Observations are consistent with the primordial density perturbations being entirely adiabatic, providing key support for inflation, and ruling out many models of structure formation involving, for example, cosmic strings.