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Paper   IPM / Particles%20And%20Accelerator / 16020
School of Particles and Accelerator
  Title:   Generalization of Bantilan-Ishi-Romatschke flow to Magnetohydrodynamics
  Author(s):  Masoud Shokri
  Status:   Published
  Journal: JHEP
  Year:  2019
  Pages:   30
  Supported by:  IPM
  Abstract:
We present a generalization of the Bantilan-Ishi-Romatschke (BIR) solution of relativistic hydrodynamics to relativistic magnetohydrodynamics (RMHD). Using the symmetries of the boundary of the Kerr-AdS5 black hole, and certain simplifying assumptions we solve the equations of RMHD on this boundary for a highly conductive fluid. We then transform the resulting solution to the flat spacetime. Furthermore, we show that the force-free condition causes the magnetic field to become singular at particular points and propose a regularization process for removing the singularities. The regularization process reveals the importance of non-vanishing electrical current in RMHD.

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