
TL;DR
This paper develops a framework for defining chiral fermions in curved spacetime, enabling direct computation of anomalies without weak field assumptions.
Contribution
It introduces a locally covariant approach to chiral fermions, allowing anomaly calculations on non-compact Lorentzian manifolds.
Findings
Explicit computation of chiral anomalies in curved backgrounds
Framework applicable to non-compact Lorentzian spacetimes
Avoids weak field approximation in anomaly calculations
Abstract
We define chiral fermions in the presence of non-trivial gravitational and gauge background fields in the framework of locally covariant field theory. This allows to straightforwardly compute the chiral anomalies on non-compact Lorentzian space-times, without recourse to a weak field approximation.
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