Abstract
In this paper we revisit the variable star phenomenon using the generalized Boltzmann kinetics theory. The main goals of investigations realized in the paper consist in answer two questions: A) Is it possible to construct the self-consistent non-local theory of explosion after the initial perturbation with taking into account the possible turbulent fluctuations? B) Is it possible to take into account the effect of the gravitational self-catching leading to periodic star pulsations? Both questions have the positive answers.
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