Path integral analysis of the axial anomaly in very special relativity

dc.creator	Bufalo, R.
dc.creator	Ghasemkhani, M.
dc.date.accessioned	2022-07-08T15:23:52Z
dc.date.available	2022-07-08T15:23:52Z
dc.date.issued	2022-01-19
dc.description.abstract	In this note, we revise the problem of the axial anomaly in the framework of Very Special Relativity following Fujikawa’s path integral approach. We show nonperturbatively that no VSR contribution is present in the path integral measure in (3 + 1)-dimensional spacetime. Furthermore, we extend our results to (1 + 1) dimensions, as well as to the two-dimensional curved spacetime.	pt_BR
dc.identifier.citation	BUFALO, R.; GHASEMKHANI, M. Path integral analysis of the axial anomaly in very special relativity. Modern Physics Letters A, [S.l.], v. 37, n. 1, 2022. DOI: 10.1142/S021773232250002X.	pt_BR
dc.identifier.uri	https://repositorio.ufla.br/handle/1/50505
dc.identifier.uri	https://www.worldscientific.com/doi/abs/10.1142/S021773232250002X	pt_BR
dc.language	en_US	pt_BR
dc.publisher	World Scientific Publishing	pt_BR
dc.rights	openAccess	pt_BR
dc.source	Modern Physics Letters A	pt_BR
dc.subject	Axial anomaly	pt_BR
dc.subject	Fujikawa’s path integral	pt_BR
dc.subject	Very special relativity (VSR)	pt_BR
dc.title	Path integral analysis of the axial anomaly in very special relativity	pt_BR
dc.type	Artigo	pt_BR

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