An, F. P.Bai, W. D.Balantekin, A. B.Bishai, M.Blyth, S.Cao, G. F.Cao, J.Chang, J. F.Chang, Y.Chen, H. S.Chen, H. Y.Chen, S. M.Chen, Y.Chen, Y. X.Cheng, J.Cheng, J.Cheng, Y. -C.Cheng, Z. K.Cherwinka, J. J.Chu, M. C.Cummings, J. P.Dalager, O.Deng, F. S.Ding, Y. Y.Diwan, M. V.Dohnal, T.Dolzhikov, D.Dove, J.Dugas, K. V.Duyang, H. Y.Dwyer, D. A.Gallo, J. P.Gonchar, M.Gong, G. H.Gong, H.Gu, W. Q.Guo, J. Y.Guo, L.Guo, X. H.Guo, Y. H.Guo, Z.Hackenburg, R. W.Han, Y.Hans, S.He, M.Heeger, K. M.Heng, Y. K.Hor, Y. K.Hsiung, Y. B.Hu, B. Z.Hu, J. R.Hu, T.Hu, Z. J.Huang, H. X.Huang, J. H.Huang, X. T.Huang, Y. B.Huber, P.Jaffe, D. E.Jen, K. L.Ji, X. L.Ji, X. P.Johnson, R. A.Jones, D.Kang, L.Kettell, S. H.Kohn, S.Kramer, M.Langford, T. J.Lee, J.Lee, J. H. C.Lei, R. T.Leitner, R.Leung, J. K. C.Li, F.Li, H. L.Li, J. J.Li, Q. J.Li, R. H.Li, S.Li, S. C.Li, W. D.Li, X. N.Li, X. Q.Li, Y. F.Li, Z. B.Liang, H.Lin, C. J.Lin, G. L.Lin, S.Ling, J. J.Link, Jonathan M.Littenberg, L.Littlejohn, B. R.Liu, J. C.Liu, J. L.Liu, J. X.Lu, C.Lu, H. Q.Luk, K. B.Ma, B. Z.Ma, X. B.Ma, X. Y.Ma, Y. Q.Mandujano, R. C.Marshall, C.McDonald, K. T.McKeown, R. D.Meng, Y.Napolitano, J.Naumov, D.Naumova, E.Nguyen, T. M. T.Ochoa-Ricoux, J. P.Olshevskiy, A.Park, J.Patton, S.Peng, J. C.Pun, C. S. J.Qi, F. Z.Qi, M.Qian, X.Raper, N.Ren, J.Reveco, C. MoralesRosero, R.Roskovec, B.Ruan, X. C.Russell, B.Steiner, H.Sun, J. L.Tmej, T.Treskov, K.Tse, W. -H.Tull, C. E.Tung, Y. C.Viren, B.Vorobel, V.Wang, C. H.Wang, J.Wang, M.Wang, N. Y.Wang, R. G.Wang, W.Wang, X.Wang, Y.Wang, Y. F.Wang, Z.Wang, Z.Wang, Z. M.Wei, H. Y.Wei, L. H.Wen, L. J.Whisnant, K.White, C. G.Wong, H. L. H.Worcester, E.Wu, D. R.Wu, Q.Wu, W. J.Xia, D. M.Xie, Z. Q.Xing, Z. Z.Xu, H. K.Xu, J. L.Xu, T.Xue, T.Yang, C. G.Yang, L.Yang, Y. Z.Yao, H. F.Ye, M.Yeh, M.Young, B. L.Yu, H. Z.Yu, Z. Y.Yue, B. B.Zavadskyi, V.Zeng, S.Zeng, Y.Zhan, L.Zhang, C.Zhang, F. Y.Zhang, H. H.Zhang, J. L.Zhang, J. W.Zhang, Q. M.Zhang, S. Q.Zhang, X. T.Zhang, Y. M.Zhang, Y. X.Zhang, Y. Y.Zhang, Z. J.Zhang, Z. P.Zhang, Z. Y.Zhao, J.Zhao, R. Z.Zhou, L.Zhuang, H. L.Zou, J. H.2024-01-222024-01-222023-05-220031-9007https://hdl.handle.net/10919/117534Reactor neutrino experiments play a crucial role in advancing our knowledge of neutrinos. In this Letter, the evolution of the flux and spectrum as a function of the reactor isotopic content is reported in terms of the inverse-beta-decay yield at Daya Bay with 1958 days of data and improved systematic uncertainties. These measurements are compared with two signature model predictions: the Huber-Mueller model based on the conversion method and the SM2018 model based on the summation method. The measured average flux and spectrum, as well as the flux evolution with the Pu239 isotopic fraction, are inconsistent with the predictions of the Huber-Mueller model. In contrast, the SM2018 model is shown to agree with the average flux and its evolution but fails to describe the energy spectrum. Altering the predicted inverse-beta-decay spectrum from Pu239 fission does not improve the agreement with the measurement for either model. The models can be brought into better agreement with the measurements if either the predicted spectrum due to U235 fission is changed or the predicted U235, U238, Pu239, and Pu241 spectra are changed in equal measure.8 page(s)application/pdfenCreative Commons Attribution 4.0 InternationalPhysicsDaya Bay CollaborationNuclear ReactorsUraniumArticle - Refereedhttps://doi.org/10.1103/PhysRevLett.130.21180113021Link, Jonathan [0000-0002-1514-0650]372950751079-7114