Standard Model Anomalies in Curved Space-Time with Torsion

dc.creatorDobado, Antonio
dc.creatorMaroto, Antonio L.
dc.date1995-09-05
dc.date.accessioned2026-07-07T12:03:14Z
dc.date.available2026-07-07T12:03:14Z
dc.descriptionUsing the Fujikawa and the heat-kernel methods we make a complete and detailed computation of the global, gauge and gravitational anomalies present in the Standard Model defined on a curved space time with torsion. We find new contributions coming from curvature and torsion terms to the leptonic number anomaly (so that $B-L$ is not conserved any more), to the $U(1)_Y$ gauge and to the mixed $U(1)_Y$-gravitational anomalies, but the gauge anomaly cancellation conditions on the hypercharges remain the same. We also find that the condition, usually related to the cancellation of the mixed $U(1)_Y$-gravitational anomaly, can be reobtained in the context of the Standard Model in flat space-time by requiring the cancellation of the global Lorentz anomaly without any reference to gravitation.
dc.description44 pages, latex, no figures
dc.identifierhttps://arxiv.org/abs/hep-ph/9509227
dc.identifierhttp://arxiv.org/abs/hep-ph/9509227
dc.identifierPhys.Rev.D54:5185-5194,1996
dc.identifierdoi:10.1103/PhysRevD.54.5185
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/207713
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleStandard Model Anomalies in Curved Space-Time with Torsion
dc.typetext

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