Unified generalized model of Dynamo and transient flow generation in Stellar Atmospheres

In present thesis we investigated the flow acceleration and magnetic field generation phenomena in atmospheres of compact stars with degenerate electrons based on quasi-equilibrium approach developed in [1]. The obtained parameters will later constitute the equilibrium state-characteristic values to study the Unified generalized model of Dynamo/Reverse Dynamo [2] and transient flow generation in such environments. In our study classical gravity is included as well as electron-ion plasma with degenerate electrons is taken compressible. We assumed that there exist fully ionized and magnetized plasma structures at some height so that the quasi-equilibrium two-fluid model will capture the essential physics of flow acceleration/generation. We found, that there is a catastrophe in the system. Following are the significant results obtained throughout the study: finding the appropriate physical parameter regions for flow generation/acceleration in White Dwarfs outer layers/atmospheres; dependence of the flow strength on the compactness of the layer; the possibility of the super-Alfvénic flow generation in White Dwarf outer layer; the possibility of simultaneous flow acceleration and magnetic field generation for specific parameters of the system; The possibility of transient jet formation. References [1] S.M. Mahajan, K.I. Nikol’skaya, N.L. Shatashvili and Z. Yoshida. Astrophys, J., 576, L161 (2002). [2] S.M. Mahajan, N.L. Shatashvili, S.V. Mikeladze and K.I. Sigua, Astrophys. J. 634, 419 (2005).