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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