Energy equality and uniqueness of weak solutions to MHD equations in \(L^{\infty }(0,T;L^n (\Omega ))\)
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Publication:1034304
DOI10.1007/s10114-009-7214-8zbMath1178.35307OpenAlexW2070821457MaRDI QIDQ1034304
Publication date: 11 November 2009
Published in: Acta Mathematica Sinica. English Series (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10114-009-7214-8
PDEs in connection with fluid mechanics (35Q35) Magnetohydrodynamics and electrohydrodynamics (76W05) Weak solutions to PDEs (35D30)
Related Items (6)
Note on energy equality of MHD system ⋮ Dynamic bifurcation for the granulation convection in the solar photosphere ⋮ Energy conservation and regularity for the 3D magneto-hydrodynamics equations ⋮ Energy equality of MHD system under a weaker condition on magnetic field ⋮ Pullback attractors for 2D MHD equations on time-varying domains ⋮ Pullback attractors for 2D MHD equations with delays
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- On the regularity of weak solutions to the magnetohydrodynamic equations
- L3,∞-solutions of the Navier-Stokes equations and backward uniqueness
- REMARK ON UNIQUENESS OF WEAK SOLUTIONS TO THE NAVIER-STOKES EQUATIONS
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