Microscopic origin of the chiral pressure in a two-dimensional fluid

@misc{reyes2026microscopic,
  title = {{Microscopic origin of the chiral pressure in a two-dimensional fluid}},
  author = {Francisco Vega Reyes},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.02003},
  eprint = {2610.02003},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.02003},
}

TY  - UNPB
TI  - Microscopic origin of the chiral pressure in a two-dimensional fluid
AU  - Francisco Vega Reyes
PY  - 2026
DA  - 2026/10/01
PB  - arXiv
DO  - 10.48550/arxiv.2610.02003
UR  - https://arxiv.org/abs/2610.02003
AB  - We show that a two-dimensional chiral fluid supports an antisymmetric contribution to the pressure, and determine its microscopic expression. Its origin lies outside the standard kinetic and collisional channels of the normal pressure tensor, stemming instead from the average of a parity-breaking pseudo-scalar. This chiral pressure is set by the rotational (vortex) viscosity of micropolar hydrodynamics, whose kinetic value for rough disks we compute here, to Gaussian order. Crucially, both the chiral pressure and the rotational viscosity survive at zeroth order in the gradients, meaning they persist even in the fully homogeneous fluid -- which we show is not only well defined but steady (the Quiescent Chiral State, QCS). Since this averaged pseudo-scalar does not vanish in a chiral fluid, any expansion of its distribution function must contain terms in this pseudo-scalar variable.
ER  -