Skip to main page content
U.S. flag

An official website of the United States government

Dot gov

The .gov means it’s official.
Federal government websites often end in .gov or .mil. Before sharing sensitive information, make sure you’re on a federal government site.

Https

The site is secure.
The https:// ensures that you are connecting to the official website and that any information you provide is encrypted and transmitted securely.

Access keys NCBI Homepage MyNCBI Homepage Main Content Main Navigation
. 2023 May 26;130(21):211801.
doi: 10.1103/PhysRevLett.130.211801.

Improved Measurement of the Evolution of the Reactor Antineutrino Flux and Spectrum at Daya Bay

F P An  1 W D Bai  1 A B Balantekin  2 M Bishai  3 S Blyth  4 G F Cao  5 J Cao  5 J F Chang  5 Y Chang  6 H S Chen  5 H Y Chen  7 S M Chen  7 Y Chen  1   8 Y X Chen  9 J Cheng  9 J Cheng  9 Y-C Cheng  4 Z K Cheng  1 J J Cherwinka  2 M C Chu  10 J P Cummings  11 O Dalager  12 F S Deng  13 Y Y Ding  5 M V Diwan  3 T Dohnal  14 D Dolzhikov  15 J Dove  16 K V Dugas  12 H Y Duyang  17 D A Dwyer  18 J P Gallo  19 M Gonchar  15 G H Gong  7 H Gong  7 W Q Gu  3 J Y Guo  1 L Guo  7 X H Guo  20 Y H Guo  21 Z Guo  7 R W Hackenburg  3 Y Han  1 S Hans  3 M He  5 K M Heeger  22 Y K Heng  5 Y K Hor  1 Y B Hsiung  4 B Z Hu  4 J R Hu  5 T Hu  5 Z J Hu  1 H X Huang  23 J H Huang  5 X T Huang  17 Y B Huang  24 P Huber  25 D E Jaffe  3 K L Jen  26 X L Ji  5 X P Ji  3 R A Johnson  27 D Jones  28 L Kang  29 S H Kettell  3 S Kohn  30 M Kramer  18   30 T J Langford  22 J Lee  18 J H C Lee  31 R T Lei  29 R Leitner  14 J K C Leung  31 F Li  5 H L Li  5 J J Li  7 Q J Li  5 R H Li  5 S Li  29 S C Li  25 W D Li  5 X N Li  5 X Q Li  32 Y F Li  5 Z B Li  1 H Liang  13 C J Lin  18 G L Lin  26 S Lin  29 J J Ling  1 J M Link  25 L Littenberg  3 B R Littlejohn  19 J C Liu  5 J L Liu  33 J X Liu  5 C Lu  34 H Q Lu  5 K B Luk  18   30   35 B Z Ma  17 X B Ma  9 X Y Ma  5 Y Q Ma  5 R C Mandujano  12 C Marshall  18 K T McDonald  34 R D McKeown  36   37 Y Meng  33 J Napolitano  28 D Naumov  15 E Naumova  15 T M T Nguyen  26 J P Ochoa-Ricoux  12 A Olshevskiy  15 J Park  25 S Patton  18 J C Peng  16 C S J Pun  31 F Z Qi  5 M Qi  38 X Qian  3 N Raper  1 J Ren  23 C Morales Reveco  12 R Rosero  3 B Roskovec  14 X C Ruan  23 B Russell  18 H Steiner  18   30 J L Sun  39 T Tmej  14 K Treskov  15 W-H Tse  10 C E Tull  18 Y C Tung  4 B Viren  3 V Vorobel  14 C H Wang  6 J Wang  1 M Wang  17 N Y Wang  20 R G Wang  5 W Wang  1   37 X Wang  40 Y Wang  38 Y F Wang  5 Z Wang  5 Z Wang  7 Z M Wang  5 H Y Wei  3 L H Wei  5 L J Wen  5 K Whisnant  41 C G White  19 H L H Wong  18   30 E Worcester  3 D R Wu  5 Q Wu  17 W J Wu  5 D M Xia  42 Z Q Xie  5 Z Z Xing  5 H K Xu  5 J L Xu  5 T Xu  7 T Xue  7 C G Yang  5 L Yang  29 Y Z Yang  7 H F Yao  5 M Ye  5 M Yeh  3 B L Young  41 H Z Yu  1 Z Y Yu  5 B B Yue  1 V Zavadskyi  3   15 S Zeng  5 Y Zeng  1 L Zhan  5 C Zhang  3 F Y Zhang  33 H H Zhang  1 J L Zhang  38 J W Zhang  5 Q M Zhang  21 S Q Zhang  1 X T Zhang  5 Y M Zhang  1 Y X Zhang  39 Y Y Zhang  33 Z J Zhang  29 Z P Zhang  13 Z Y Zhang  5 J Zhao  5 R Z Zhao  5 L Zhou  5 H L Zhuang  5 J H Zou  5 Daya Bay Collaboration
Affiliations

Improved Measurement of the Evolution of the Reactor Antineutrino Flux and Spectrum at Daya Bay

F P An et al. Phys Rev Lett. .

Abstract

Reactor 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 ^{239}Pu 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 ^{239}Pu 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 ^{235}U fission is changed or the predicted ^{235}U, ^{238}U, ^{239}Pu, and ^{241}Pu spectra are changed in equal measure.

PubMed Disclaimer

LinkOut - more resources