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- CGHS_model abstract "The Callan–Giddings–Harvey–Strominger model or CGHS in short is a toy model of general relativity in 1 spatial and 1 time dimension. General relativity is a highly nonlinear model, and as such, its 3+1D version is usually too complicated to analyze in detail. In 3+1D and higher, propagating gravitational waves exist, but not in 2+1D or 1+1D. In 2+1D, general relativity becomes a topological field theory with no local degrees of freedom, and all 1+1D models are locally flat. However, a slightly more complicated generalization of general relativity which includes dilatons will turn the 2+1D model into one admitting mixed propagating dilaton-gravity waves, as well as making the 1+1D model geometrically nontrivial locally. The 1+1D model still does not admit any propagating gravitational (or dilaton) degrees of freedom, but with the addition of matter fields, it becomes a simplified, but still nontrivial model. With other numbers of dimensions, a dilaton-gravity coupling can always be rescaled away by a conformal rescaling of the metric, converting the Jordan frame to the Einstein frame. But not in two dimensions, because the conformal weight of the dilaton is now 0. The metric in this case is more amenable to analytical solutions than the general 3+1D case. And of course, 0+1D models cannot capture any nontrivial aspect of relativity because there is no space at all.This class of models retains just enough complexity to include among its solutions black holes, their formation, FRW cosmological models, gravitational singularities, etc. In the quantized version of such models with matter fields, Hawking radiation also shows up, just as in higher-dimensional models.".
- CGHS_model wikiPageID "30268344".
- CGHS_model wikiPageRevisionID "603814291".
- CGHS_model hasPhotoCollection CGHS_model.
- CGHS_model subject Category:General_relativity.
- CGHS_model subject Category:Quantum_gravity.
- CGHS_model comment "The Callan–Giddings–Harvey–Strominger model or CGHS in short is a toy model of general relativity in 1 spatial and 1 time dimension. General relativity is a highly nonlinear model, and as such, its 3+1D version is usually too complicated to analyze in detail. In 3+1D and higher, propagating gravitational waves exist, but not in 2+1D or 1+1D. In 2+1D, general relativity becomes a topological field theory with no local degrees of freedom, and all 1+1D models are locally flat.".
- CGHS_model label "CGHS model".
- CGHS_model label "Modelo de CGHS".
- CGHS_model sameAs Modelo_de_CGHS.
- CGHS_model sameAs m.0g57_sn.
- CGHS_model sameAs Q5010970.
- CGHS_model sameAs Q5010970.
- CGHS_model wasDerivedFrom CGHS_model?oldid=603814291.
- CGHS_model isPrimaryTopicOf CGHS_model.