Gravitational corrections to the Euler-Heisenberg Lagrangian

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dc.creatorBastianelli, Fiorenzo
dc.creatorDavila, Jose Manuel
dc.creatorSchubert, Christian
dc.date2008-12-28
dc.date.accessioned2026-07-07T12:53:28Z
dc.date.available2026-07-07T12:53:28Z
dc.descriptionWe use the worldline formalism for calculating the one-loop effective action for the Einstein-Maxwell background induced by charged scalars or spinors, in the limit of low energy and weak gravitational field but treating the electromagnetic field nonperturbatively. The effective action is obtained in a form which generalizes the standard proper-time representation of the Euler-Heisenberg Lagrangian. We compare with previous work and discuss possible applications.
dc.description33 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/0812.4849
dc.identifierhttp://arxiv.org/abs/0812.4849
dc.identifierJHEP 0903:086,2009
dc.identifierdoi:10.1088/1126-6708/2009/03/086
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/223635
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGravitational corrections to the Euler-Heisenberg Lagrangian
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