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Second-order partition function of a non-interacting chiral fluid in 3+1 dimensions

We compute the partition function for non-interacting chiral fermions at second order in a derivative expansion of an arbitrary time-independent gravitational and gauge background. We find that Pauli-Villars regularization of the vacuum part is needed to get consistent results. We use our results to discuss some features of the non-dissipative constitutive relations of second order hydrodynamics.

preprint2014arXivOpen access
Eugenio MegiasManuel Valle
hep-phhep-th
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Eugenio MegiasManuel Valle

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