Self-consistent solution to the back-reaction problem for vector fields in two dimensions
We describe vector fields propagating in a two-dimensional spatially flat Robertson-Walker background using a curved space-time generalization of the Stueckelberg formalism. We prove that the energy-momentum tensor expectation value in the vacuum defined through energy minimization is renormalizable...
Guardado en:
| Autores principales: | Chimento, Luis Pascual, Cossarini, Adriana E. |
|---|---|
| Publicado: |
1992
|
| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05503213_v373_n2_p438_Chimento http://hdl.handle.net/20.500.12110/paper_05503213_v373_n2_p438_Chimento |
| Aporte de: |
Ejemplares similares
-
Self-consistent solution to the back-reaction problem for vector fields in two dimensions
por: Chimento, L.P., et al. -
Self-consistent solutions of the semi-classical back-reaction equations with cosmological constant spatial curvature and perfect fluid
por: Chimento, Luis Pascual, et al.
Publicado: (1994) -
Self-consistent solutions of the semi-classical back-reaction equations with cosmological constant spatial curvature and perfect fluid
por: Chimento, L.P., et al. -
Self-consistent solutions of the semiclassical Einstein equations with cosmological constant
por: Chimento, Luis Pascual
Publicado: (1993) -
Renormalized evolution equations for the back-reaction problem with a self-interacting scalar field
Publicado: (1988)