The PROSPECT Physics Program
J. Ashenfelter,A. B. Balantekin,H. R. Band,G. Barclay,C.D. Bass,D. Berish,Lindsey J. Bignell,Nathaniel Bowden,A. Bowes,J. P. Brodsky,C. D. Bryan,J. J. Cherwinka,Rui-Lin Chu,Rui-Lin Chu,T. Classen,K. Commeford,A. J. Conant,D. Davee,D. J. Dean,G. Deichert,M. V. Diwan,M. J. Dolinski,J. Dolph,M DuVernois,Anna Erickson,Michael Febbraro,J. K. Gaison,A. Galindo-Uribarri,A. Galindo-Uribarri,K. Gilje,A. Glenn,B. W. Goddard,M. P. Green,B. Hackett,B. Hackett,Ke Han,Ke Han,S. Hans,K. M. Heeger,B. Heffron,B. Heffron,J. Insler,D. E. Jaffe,D. C. Jones,T. J. Langford,B. R. Littlejohn,D. A. Martinez Caicedo,J. T. Matta,R D McKeown,M P Mendenhall,P. E. Mueller,Hans P. Mumm,Jim Napolitano,R. Neilson,J. Nikkel,D. Norcini,Dmitry A. Pushin,Xin Qian,E. Romero,E. Romero,Richard Rosero,B. Seilhan,R. Sharma,Steven Sheets,P. T. Surukuchi,C. Trinh,R. L. Varner,B. Viren,Wei Wang,Wei Wang,B. R. White,Christopher G. White,J. Wilhelmi,Christopher B. Williams,T. Wise,H. Yao,Minfang Yeh,Y-R Yen,G. Zangakis,Chao Zhang,X. Zhang +80 more
TL;DR: The Precision Reactor Oscillation and Spectrum Experiment (PROSPECT) as discussed by the authors was designed to make a precise measurement of the antineutrino spectrum from a highly-enriched uranium reactor and probe eV-scale sterile neutrinos by searching for neutrino oscillations over meter-long distances.
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Abstract: The Precision Reactor Oscillation and Spectrum Experiment, PROSPECT, is
designed to make a precise measurement of the antineutrino spectrum from a
highly-enriched uranium reactor and probe eV-scale sterile neutrinos by
searching for neutrino oscillations over meter-long distances. PROSPECT is
conceived as a 2-phase experiment utilizing segmented $^6$Li-doped liquid
scintillator detectors for both efficient detection of reactor antineutrinos
through the inverse beta decay reaction and excellent background
discrimination. PROSPECT Phase I consists of a movable 3-ton antineutrino
detector at distances of 7 - 12 m from the reactor core. It will probe the
best-fit point of the $\nu_e$ disappearance experiments at 4$\sigma$ in 1 year
and the favored region of the sterile neutrino parameter space at $>$3$\sigma$
in 3 years. With a second antineutrino detector at 15 - 19 m from the reactor,
Phase II of PROSPECT can probe the entire allowed parameter space below 10
eV$^{2}$ at 5$\sigma$ in 3 additional years. The measurement of the reactor
antineutrino spectrum and the search for short-baseline oscillations with
PROSPECT will test the origin of the spectral deviations observed in recent
$\theta_{13}$ experiments, search for sterile neutrinos, and conclusively
address the hypothesis of sterile neutrinos as an explanation of the reactor
anomaly.
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Figures
![Figure 1. Comparison of measured reactor antineutrino fluxes with predictions based on models for the emission of reactor antineutrinos. The measured deficit relative to prediction is known as the “reactor antineutrino anomaly” [3]. Reprinted figure with permission from [6] Copyright 2016 by the American Physical Society.](/figures/figure-1-comparison-of-measured-reactor-antineutrino-fluxes-2mm93154.png)
Figure 1. Comparison of measured reactor antineutrino fluxes with predictions based on models for the emission of reactor antineutrinos. The measured deficit relative to prediction is known as the “reactor antineutrino anomaly” [3]. Reprinted figure with permission from [6] Copyright 2016 by the American Physical Society. 
Figure 14. Comparison between unloaded EJ-309 and three different LiLS formulations. (Left) Response to 60Co, demonstrating the relative light yield. (Right) Comparison of PSD distributions when exposed to 252Cf. Li-EJ309 has the best performance amongst Li-loaded materials. 
Figure 15. (Left) Measured PE spectra including the Compton edge of 60Co and 217Bi γ-rays and the quenched (n, Li) capture peak from 252Cf neutron source. (Right) PSD performance of Li-EJ309. The upper band is neutron-like events with (n,Li) captures at ≈ 0.6 MeV dominating the statistics. The lower band shows γ-like events. 
Table 1. Nominal PROSPECT experimental parameters. Phase I consists of operating AD-I for three years split between front, middle, and back positions. Phase II adds AD-II at a longer baseline and operates both detectors for three additional years. ![Figure 2. Comparison of the detected prompt energy spectrum observed by Daya Bay to a model-based prediction of pressurized water reactor (PWR) neutrino emission. The deviation from prediction between 4–6 MeV, which is also observed in two other similar experiments, is unexplained and may indicate deficiencies in the models and/or the nuclear data underlying them. Reprinted figure with permission from [6] Copyright 2016 by the American Physical Society.](/figures/figure-2-comparison-of-the-detected-prompt-energy-spectrum-18416agm.png)
Figure 2. Comparison of the detected prompt energy spectrum observed by Daya Bay to a model-based prediction of pressurized water reactor (PWR) neutrino emission. The deviation from prediction between 4–6 MeV, which is also observed in two other similar experiments, is unexplained and may indicate deficiencies in the models and/or the nuclear data underlying them. Reprinted figure with permission from [6] Copyright 2016 by the American Physical Society. 
Figure 18. Simulated response to 4 MeV e+ for AD-I configurations with no inactive mass (red), the PROSPECT low mass optical separators (blue), and an inactive mass fraction equivalent to Bugey 3 (green).
Citations
Neutrinoless Double Beta Decay: 2015 Review
TL;DR: The discovery of neutrino masses through the observation of oscillations boosted the importance of neutrinoless double beta decay as mentioned in this paper, underlining its key role from both the experimental and theoretical point of view.
Updated Global 3+1 Analysis of Short-BaseLine Neutrino Oscillations
TL;DR: In this article, an updated fit of short-baseline neutrino oscillation data in the framework of 3+1 active-sterile neutrinos mixing is presented.
Updated Global 3+1 Analysis of Short-BaseLine Neutrino Oscillations
TL;DR: In this article, an updated fit of short-baseline neutrino oscillation data in the framework of 3+1 active-sterile neutrinos mixing is presented.
First Search for Short-Baseline Neutrino Oscillations at HFIR with PROSPECT.
J. Ashenfelter,A. B. Balantekin,C. Baldenegro,H. R. Band,C. D. Bass,Denis E. Bergeron,D. Berish,Lindsey J. Bignell,Nathaniel Bowden,J. Bricco,J. P. Brodsky,C. D. Bryan,A. Bykadorova Telles,J. J. Cherwinka,T. Classen,K. Commeford,A. J. Conant,Andrew A. Cox,D. Davee,D. J. Dean,G. Deichert,M. V. Diwan,M. J. Dolinski,Anna Erickson,Michael Febbraro,B. T. Foust,J. K. Gaison,A. Galindo-Uribarri,C. E. Gilbert,K. Gilje,A. Glenn,B. W. Goddard,B. T. Hackett,Ke Han,S. Hans,A. B. Hansell,K. M. Heeger,B. Heffron,J. Insler,D. E. Jaffe,X. Ji,D. C. Jones,K. Koehler,O. Kyzylova,C. E. Lane,T. J. Langford,J. LaRosa,B. R. Littlejohn,F. Lopez,Xin Lu,D. A. Martinez Caicedo,J. T. Matta,R. D. McKeown,M. P. Mendenhall,H. J. Miller,J. M. Minock,P. E. Mueller,Hans P. Mumm,Jim Napolitano,R. Neilson,J. A. Nikkel,D. Norcini,S. Nour,Dmitry A. Pushin,Xin Qian,E. Romero-Romero,R. Rosero,Dusan Sarenac,B. Seilhan,R. Sharma,P. T. Surukuchi,C. Trinh,M. A. Tyra,R. L. Varner,B. Viren,J. M. Wagner,Wei Wang,B. R. White,Christopher G. White,J. Wilhelmi,T. Wise,H. Yao,Minfang Yeh,Y-R Yen,Aiwu Zhang,Chao Zhang,X. Zhang,M. Zhao +87 more
TL;DR: The first scientific results from the observation of antineutrinos emitted by fission products of U at the High Flux Isotope Reactor were reported in this paper.
162
•Journal Article
Measurement of the Reactor Antineutrino Flux and Spectrum at Daya Bay
TL;DR: A measurement of the flux and energy spectrum of electron antineutrinos from six 2.9 GWth nuclear reactors with six detectors deployed in two near and far underground experimental halls in the Daya Bay experiment finds the measured IBD positron energy spectrum deviates from both spectral predictions by more than 2σ over the full energy range.
137
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