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Effects of metal abundances on the evolutionary period changes of classical Cepheids
Authors:Masaya Saitou
Institution:(1) Institute of Astrophysics, Tadjik Academy of Science, Dushanbe, U.S.S.R.
Abstract:Some peculiarities in the behaviour of a model self-gravitating system described by hydrodynamical equations and isothermal equation of state connected with the presence of thermodynamical fluctuations in real systems were investigated in numerical experiment. The values of density and velocity sgr, ngr, respectively, were computed by numerical code perturbed on each time-step and in each computational cell by random values deltasgr, deltangr for modeling such fluctuations. Perturbed values tau i prime = tau i + deltatau i ,v i prime = i + deltav i were used to initiate the next step of computations. This procedure is equivalent to an introduction into original hydrodynamical equations of Langevin sources which are random functions. It is shown that these small fluctuations (langdeltataurang= langdeltavrang =0,langdeltatau2rang =langdeltav 2rang = 10–8) grow many times in marginally-stable state.
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