In this paper, we elaborated a spectral collocation method based on differentiated Chebyshev polynomials to obtain numerical solutions for some different kinds of nonlinear partial differential equations. The problem is reduced to a system of ordinary differential equations that are solved by Runge-Kutta method of order four. Numerical results for the nonlinear evolution equations such as 1D Burgers', KdV-Burgers', coupled Burgers', 2D Burgers' and system of 2D Burgers' equations are obtained. The numerical results are found to be in good agreement with the exact solutions. Numerical computations for a wide range of values of Reynolds' number, show that the present method offers better accuracy in comparison with other previous methods. Moreover the method can be applied to a wide class of nonlinear partial differential equations.
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.
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