Abstract
We investigate the large time behavior of solutions to the equations of the MHD micropolar fluids in Sobolev spaces Hm(Rn), with n=2 or 3. More precisely, we show that â(Dmu,Dmw,Dmb)(â ,t)âL2(Rn)â€C(t+1)âm2ân4 for all tâ«1. Furthermore, we prove a faster decay estimate for the micro-rotation, namely âDmw(â ,t)âL2(Rn)â€C(t+1)âm2ân4â12 for every tâ«1. It is also shown that â(u,w,b)(â ,t)â(uâŸ,wâŸ,bâŸ)(â ,t)âL2(Rn)â€C(t+1)ân4â12 and âw(â ,t)âwâŸ(â ,t)âL2(Rn)â€C(t+1)ân4â1 for any tâ„0, where (uâŸ,wâŸ,bâŸ) is the solution to the related linear system with the same initial data. We also present some related results, e.g., decay rates for the total pressure of the fluid and space-time derivatives estimates.
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