Derives entropy covector field for relativistic kinetic gases around Schwarzschild black hole and compares rotating versus non-rotating models, finding angular momentum alters asymptotic behavior of anisotropy, temperature, and pressure.
Chemin, A mass-velocity anisotropy relation in galactic stellar disks, Astronomy & Astrophysics618, 19 (2018)
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Entropy covector field and macroscopic observables for rotating and non-rotating relativistic kinetic gases around a Schwarzschild black hole
Derives entropy covector field for relativistic kinetic gases around Schwarzschild black hole and compares rotating versus non-rotating models, finding angular momentum alters asymptotic behavior of anisotropy, temperature, and pressure.