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Fundamentals of the Mechanics of a Turbulent Gas and Dust Medium for an Accretion Protoplanetary Disk

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Abstract—In this paper, in relation to the problem of reconstructing the evolution of a preplanetary gas and dust cloud, an attempt is made to develop a model of a turbulent heterogeneous medium and to construct on this basis a new class of mathematical models of space media that take into how the character and development of turbulence are influenced by the inertial properties of a polydisperse mixture of dust particles, processes of heat and mass transfer and coagulation, phase transitions, chemical reactions, and radiation. This can significantly expand the capabilities of numerical modeling of various physical phenomena in complex space media such as accretion gas and dust disks formed in stars of various classes during their differential rotation around the center of gravity, to study their structure, physicochemical and hydrodynamic properties, and time evolution.

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    A. V. Kolesnichenko

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Kolesnichenko, A.V. Fundamentals of the Mechanics of a Turbulent Gas and Dust Medium for an Accretion Protoplanetary Disk. Sol Syst Res 57, 655–705 (2023). https://doi.org/10.1134/S0038094623070043

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