Nonlinear Alfvén waves, propagating along a homogeneous
magnetic field, are studied using relativistic isotropic
hydrodynamics. Alfvén solitons of the moving-wave and wave
packet types are considered for modified Korteweg–de Vries
(mKdV) equation and the nonlinear Schrödinger (NLS) equation,
respectively. The method of characteristics is used and the
Bäcklund transformations (BTs) are employed to generate new
solutions from the old ones. Thus, families of new solutions for the
mKdV and the NLS equations are obtained. The question arises which
solitons exist in the pulsar atmosphere.
The motion of non-Newtonian fluid with heat and mass transfer through porous medium past a shrinking plate is discussed. The fluid obeys Casion model, heat generation, viscous dissipation, thermal diffusion and chemical reaction are taken in our considered. The motion is modulated mathematically by a system of non liner partial differential equations which describe the continuity, momentum, heat and mass equations. These system of non linear equations are transformed into ordinary differential equations by using a suitable transformations. These equations are solved numerically by using Mathematica package. The numerical distributions of the velocity, temperature and concentration are obtained as a functions of the physical parameters of the problem. Moreover the effects of these parameters on these solutions are discussed numerically and illustrated graphically through some figures. It is clear that these parameters play an important role to control the velocity, temperature and concentration of the fluid motion. It's found that the fluid velocity deceases with the increasing of electric parameter while it increases as the magnetic hartman parameter increases, these results is good agreament with the physical sitution. Also, the fluid temperature decreases and increases as the Prandtl number and Eckert number increases respeictively. At least the fluid concentration decreases with both of soret and schimdt numbers.
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