# Dark energy or apparent acceleration due to a relativistic cosmological model more complex than the Friedmann-Lemaitre-Robertson-Walker model?

@article{Ishak2008DarkEO, title={Dark energy or apparent acceleration due to a relativistic cosmological model more complex than the Friedmann-Lemaitre-Robertson-Walker model?}, author={Mustapha Ishak and James A. Richardson and David Garred and Delilah Whittington and Anthony Nwankwo and Roberto Sussman}, journal={Physical Review D}, year={2008}, volume={78}, pages={123531} }

We use the Szekeres inhomogeneous relativistic models in order to fit supernova combined data sets. We show that with a choice of the spatial curvature function that is guided by current observations, the models fit the supernova data almost as well as the Lambda-CDM model without requiring a dark energy component. The Szekeres models were originally derived as an exact solution to Einstein's equations with a general metric that has no symmetries, and they are regarded as good candidates to… Expand

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