We investigate the recent Daya Bay results on the changes in the antineutrino flux and spectrum with the burnup of the reactor fuel. We find that the discrepancy between current model predictions and the Daya Bay results can be traced to the original measured 235 U/ 239 Pu ratio of the fission beta spectra that were used as a base for the expected antineutrino fluxes. An analysis of the antineutrino spectra that is based on a summation over all fission fragment beta-decays, using nuclear database input, explains all of the features seen in the Daya Bay evolution data. However, this summation method still predicts an anomaly. Thus, we conclude that there is currently not enough information to use the antineutrino flux changes to rule out the possible existence of sterile neutrinos.Recent results from the Daya Bay (DB) reactor neutrino experiment [1] show significant change in the emitted antineutrino flux with the evolution of the reactor fuel. Over the course of 1230 days, the fuel evolved such that the fraction of fissions from 239 Pu increased from 25% to 35%, while those from 235 U decreased from 63% to 51%. Over the same period, the fraction from 238 U remained approximately constant at 7.6%, while the 241 Pu fraction increased from 4% to 8%. The dependence of antineutrino flux on the fuel evolution was measured [1] by the change in the yield from the inverse beta decay (IBD) reaction ν + p → e + + n with the variation in the 239 Pu fission fraction, F 239 . The IBD yield, which is an integral over energy of the product of the IBD cross section and the antineutrino flux per fission, was fitted with a linear dependence on F 239 as [1],