Analytic solutions of relativistic dissipative spin hydrodynamics with radial expansion in Gubser flow
arXiv:2112.15535 · doi:10.1103/PhysRevD.105.114050
Abstract
We have derived the analytic solutions of dissipative relativistic spin hydrodynamics with Gubser expansion. Following the standard strategy of deriving the solutions in a Gubser flow, we take the Weyl rescaling and obtain the energy-momentum and angular momentum conversation equations in the space-time. We then derive the analytic solutions of spin density, spin potential and other thermodynamic in space-time and transform them back into Minkowski space-time . In the Minkowski space-time, the spin density and spin potential including the information of radial expansion decay as and in large limit, with being proper time and being the characteristic length of the system, respectively. Moreover, we observe the non-vanishing spin corrections to the energy density and other dissipative terms in the Belinfante form of dissipative spin hydrodynamics. Our results can also be used as test beds for future simulations of relativistic dissipative spin hydrodynamics.
28 pages; 1 table and 1 figure are added
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- Foundations and Applications of Quantum Kinetic Theory
- Relativistic Spin Magnetohydrodynamics
- Lorentz-covariant nonlocal collision term for spin-1/2 particles
- Damping of spin waves
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- Finite-Density Dynamics of Chemically Equilibrating QGP in Conformal Gubser Flow and Hard Thermal Photon Production