On Torsion Contribution to Chiral Anomaly via Nieh-Yan Term
Ida M. Rasulian, Mahdi Torabian

TL;DR
This paper investigates whether the Nieh-Yan term contributes to chiral anomaly in the presence of torsion, revealing conditions under which it affects the anomaly and how it depends on spacetime and IR cut-offs.
Contribution
It demonstrates that the Nieh-Yan term's contribution to chiral anomaly depends on topology, singularities, and IR cut-offs, and introduces a quantization condition to remove ill-behaved dependencies.
Findings
Nieh-Yan term contributes to chiral anomaly with a dimensionful coefficient in certain conditions.
Singularities in the Nieh-Yan term lead to sinusoidal dependence on UV cut-off.
Contribution can be nullified if singularities are absent, making the term smoothly rotatable away.
Abstract
In this note we present a solution to the question of whether or not, in the presence of torsion, the topological Nieh-Yan term contributes to chiral anomaly. The integral of Nieh-Yan term is non-zero if topology is non-trivial; the manifold has a boundary or vierbeins have singularities. Noting that singular Nieh-Yan term could be written as a sum of delta functions, we argue that the heat kernel expansion cannot end at finite steps. This leads to a sinusoidal dependence on the Nieh-Yan term and the UV cut-off of the theory (or alternatively the minimum length of spacetime). We show this ill-behaved dependence can be removed if a quantization condition on length scales is applied. It is expected as the Nieh-Yan term can be derived as the difference of two Chern class integrals (i.e. Pontryagin terms). On the other hand, in the presence of a cosmological constant, we find that indeed…
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Taxonomy
TopicsNoncommutative and Quantum Gravity Theories · Cosmology and Gravitation Theories · Black Holes and Theoretical Physics
