Back reaction effects in black hole spacetimes
We solve the semiclassical Einstein equations for the static spherically symmetric case. Using expressions for the renormalized 〈Tμv〉, we study the effects of the back reaction on black hole spacetimes at the one-loop level. Two different situtaions appear depending on the graviton-matter balance. I...
Guardado en:
| Publicado: |
1988
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03702693_v212_n4_p411_Lousto http://hdl.handle.net/20.500.12110/paper_03702693_v212_n4_p411_Lousto |
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