Ramanujan Auditorium

Relativistic spin-(magneto) hydrodynamics

Amaresh Jaiswal

NISER Bhubaneswar

Relativistic dissipative hydrodynamics has been applied quite  successfully to understand the space-time evolution of strongly  interacting hot and dense matter formed in high energy
heavy-ion collisions. Recent relativistic heavy-ion collision experiments have also found evidence for the generation of strong magnetic fields and global angular momentum. The presence of
these effects requires us to revisit our formulation of relativistic hydrodynamics.

In this presentation, I will outline our contribution in the development of hydrodynamic formulation for evolution of a dissipative fluid having global angular momentum and in the presence
of a magnetic field. I will also discuss some applications of these formulations in the context of relativistic heavy ion collisions as well as electron hydrodynamics in graphene.