Published December 7, 2009 | Version v1
Journal article

Anomaly poles as common signatures of chiral and conformal anomalies

  • 1. Dipartimento di Fisica, Universita del Salento and INFN Sezione di Lecce, Via Arnesano, 73100 Lecce (Italy)
  • 2. Department of Physics, University of Crete, Heraklion, Crete (Greece)

Description

One feature of the chiral anomaly, analyzed in a perturbative framework, is the appearance of massless poles which account for it. They are identified by a spectral analysis of the anomaly graph and are usually interpreted as being of an infrared origin. Recent investigations show that their presence is not just confined in the infrared, but that they appear in the effective action under the most general kinematical conditions, even if they decouple in the infrared. Further studies reveal that they are responsible for the non-unitary behaviour of these theories in the ultraviolet (UV) region. We extend this analysis to the case of the conformal anomaly, showing that the effective action describing the interaction of gauge fields with gravity is characterized by anomaly poles that give the entire anomaly and are decoupled in the infrared (IR), in complete analogy with the chiral case. This complements a related analysis by Giannotti and Mottola on the trace anomaly in gravity, in which an anomaly pole has been identified in the corresponding correlator using dispersion theory in the IR. Our extension is based on an exact computation of the off-shell correlation function involving an energy-momentum tensor and two vector currents (the gauge-gauge-graviton vertex) which is responsible for the appearance of the anomaly.

Availability note (English)

Available from http://dx.doi.org/10.1016/j.physletb.2009.11.013

Additional details

Identifiers

DOI
10.1016/j.physletb.2009.11.013;
arXiv
arXiv:0909.4522v4;
PII
S0370-2693(09)01346-X;

Publishing Information

Journal Title
Physics Letters. Section B
Journal Volume
682
Journal Issue
3
Journal Page Range
p. 322-327
ISSN
0370-2693
CODEN
PYLBAJ

Optional Information

Copyright
Copyright (c) 2009 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.