%0 Generic %1 Moffat2009 %A Moffat, J. W. %D 2009 %K Dark Energy Void %T Void or Dark Energy? %U http://arxiv.org/abs/0910.2723 %X Two possible explanations for the type SNe Ia supernovae observations are a nonlinearly, underdense void embedded in a matter-dominated Einstein-de Sitter spacetime or dark energy in the $Łambda$CDM model. Both of these alternatives are faced with Copernican fine-tuning problems. A case is made for the void scenario that avoids introducing undetected dark energy.

@misc{Moffat2009, abstract = { Two possible explanations for the type SNe Ia supernovae observations are a nonlinearly, underdense void embedded in a matter-dominated Einstein-de Sitter spacetime or dark energy in the $\Lambda$CDM model. Both of these alternatives are faced with Copernican fine-tuning problems. A case is made for the void scenario that avoids introducing undetected dark energy. }, added-at = {2009-10-16T15:53:30.000+0200}, author = {Moffat, J. W.}, biburl = {https://www.bibsonomy.org/bibtex/22cf34105f8c91677b72208d5aeb3b00a/ad4}, description = {Void or Dark Energy?}, interhash = {8941ad72ae0daf0fc17d954d6a09b710}, intrahash = {2cf34105f8c91677b72208d5aeb3b00a}, keywords = {Dark Energy Void}, note = {cite arxiv:0910.2723 Comment: 22 pages, 3 figures, LaTex file la}, timestamp = {2009-10-16T15:53:30.000+0200}, title = {{V}oid or {D}ark {E}nergy?}, url = {http://arxiv.org/abs/0910.2723}, year = 2009 }