Magnetized Anisotropic Dark Energy Models in Barber’s Second Self-Creation Theory

The present paper deals with Bianchi type IX cosmological model with magnetized anisotropic dark energy by using Barber’s self-creation theory. The energy momentum tensor consists of anisotropic fluid with EoS parameter <math id="M1" xmlns="http://www.w3.org/1998/Math/MathML"><mrow><mi>ω</mi></mrow></math> and a uniform magnetic field of energy density <math id="M2" xmlns="http://www.w3.org/1998/Math/MathML"><mrow><msub><mrow><mi>ρ</mi></mrow><mrow><mi>B</mi></mrow></msub></mrow></math> . In order to obtain the exact solution we have assumed that dark energy components and the components of magnetic field interact minimally and obey the law of conservation of energy momentum tensors. We have also used the special law of variation for the mean generalized Hubble parameter and power law relation between scalar field and scale factor. Some physical and kinematical properties of the models have been discussed