Jonathan Link

Prof. Jonathan Link


Research Focus & Metrics

Academic Career Length

35Years (1992-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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23 April 2012 in Physical Review Letters
Verified
Journal Article
Open access
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FAF. P. An
F. P. An
JBJ. Z. Bai
J. Z. Bai
ABA. B. Balantekin
A. B. Balantekin
HBH. R. Band
H. R. Band
DBD. Beavis
D. Beavis
JZJ. H. Zou
J. H. Zou
The Daya Bay Reactor Neutrino Experiment has measured a nonzero value for the neutrino mixing angle θ13 with a significance of 5.2 standard deviations. Antineutrinos from six 2.9 GWth reactors were detected in six antineutrino detectors deployed in two near (flux-weighted baseline 470 m and 576 m) and one far (1648 m) underground experimental halls. With a 43 000  ton–GWth–day live-time exposure in 55 days, 10 416 (80 376) electron-antineutrino candidates were detected at the far hall (near halls). The ratio of the observed to expected number of antineutrinos at the far hall is R=0.940±0.011(stat.)±0.004(syst.). A rate-only analysis finds sin22θ13=0.092±0.016(stat.)±0.005(syst.) in a three-neutrino framework.

28 May 2010 in Physical Review D
Verified
Journal Article
Closed access
PDF file
AAA. A. Aguilar-Arevalo
A. A. Aguilar-Arevalo
CAC. E. Anderson
C. E. Anderson
ABA. O. Bazarko
A. O. Bazarko
SBS. J. Brice
S. J. Brice
BBB. C. Brown
B. C. Brown
EZE. D. Zimmerman
E. D. Zimmerman
A high-statistics sample of charged-current muon neutrino scattering events collected with the MiniBooNE experiment is analyzed to extract the first measurement of the double differential cross section (d2σdTμdcosθμ) for charged-current quasielastic (CCQE) scattering on carbon. This result features minimal model dependence and provides the most complete information on this process to date. With the assumption of CCQE scattering, the absolute cross section as a function of neutrino energy (σ[Eν]) and the single differential cross section (dσdQ2) are extracted to facilitate comparison with previous measurements. These quantities may be used to characterize an effective axial-vector form factor of the nucleon and to improve the modeling of low-energy neutrino interactions on nuclear targets. The results are relevant for experiments searching for neutrino oscillations.

8 June 2007 in Physical Review Letters
Verified
Journal Article
Closed access
PDF file
AAA. A. Aguilar-Arevalo
A. A. Aguilar-Arevalo
ABA. O. Bazarko
A. O. Bazarko
SBS. J. Brice
S. J. Brice
BBB. C. Brown
B. C. Brown
LBL. Bugel
L. Bugel
EZE. D. Zimmerman
E. D. Zimmerman
The MiniBooNE Collaboration reports first results of a search for νe appearance in a νμ beam. With two largely independent analyses, we observe no significant excess of events above the background for reconstructed neutrino energies above 475 MeV. The data are consistent with no oscillations within a two-neutrino appearance-only oscillation model.

15 April 2009 in Physical Review D
Verified
Journal Article
Closed access
PDF file
AAA. A. Aguilar-Arevalo
A. A. Aguilar-Arevalo
CAC. E. Anderson
C. E. Anderson
ABA. O. Bazarko
A. O. Bazarko
SBS. J. Brice
S. J. Brice
BBB. C. Brown
B. C. Brown
EZE. D. Zimmerman
E. D. Zimmerman
The booster neutrino experiment (MiniBooNE) searches for νμ→νe oscillations using the O(1  GeV) neutrino beam produced by the booster synchrotron at the Fermi National Accelerator Laboratory). The booster delivers protons with 8 GeV kinetic energy (8.89  GeV/c momentum) to a beryllium target, producing neutrinos from the decay of secondary particles in the beam line. We describe the Monte Carlo simulation methods used to estimate the flux of neutrinos from the beam line incident on the MiniBooNE detector for both polarities of the focusing horn. The simulation uses the Geant4 framework for propagating particles, accounting for electromagnetic processes and hadronic interactions in the beam line materials, as well as the decay of particles. The absolute double differential cross sections of pion and kaon production in the simulation have been tuned to match external measurements, as have the hadronic cross sections for nucleons and pions. The statistical precision of the flux predictions is enhanced through reweighting and resampling techniques. Systematic errors in the flux estimation have been determined by varying parameters within their uncertainties, accounting for correlations where appropriate.

11 March 2009 in Physical Review Letters
Verified
Journal Article
Closed access
PDF file
AAA A Aguilar-Arevalo
A A Aguilar-Arevalo
CAC E Anderson
C E Anderson
ABA O Bazarko
A O Bazarko
SBS J Brice
S J Brice
BBB C Brown
B C Brown
MCMiniBooNE Collaboration
MiniBooNE Collaboration
The MiniBooNE Collaboration observes unexplained electronlike events in the reconstructed neutrino energy range from 200 to 475 MeV. With 6.46×1020 protons on target, 544 electronlike events are observed in this energy range, compared to an expectation of 415.2±43.4 events, corresponding to an excess of 128.8±20.4±38.3 events. The shape of the excess in several kinematic variables is consistent with being due to either νe and ν¯e charged-current scattering or νμ neutral-current scattering with a photon in the final state. No significant excess of events is observed in the reconstructed neutrino energy range from 475 to 1250 MeV, where 408 events are observed compared to an expectation of 385.9±35.7 events.

14 December 2018 in Physical Review Letters
Verified
Journal Article
Open access
PDF file
DAD. Adey
D. Adey
FAF. P. An
F. P. An
ABA. B. Balantekin
A. B. Balantekin
HBH. R. Band
H. R. Band
MBM. Bishai
M. Bishai
TCThe Daya Bay Collaboration
The Daya Bay Collaboration
We report a measurement of electron antineutrino oscillation from the Daya Bay Reactor Neutrino Experiment with nearly 4 million reactor ν¯e inverse β decay candidates observed over 1958 days of data collection. The installation of a flash analog-to-digital converter readout system and a special calibration campaign using different source enclosures reduce uncertainties in the absolute energy calibration to less than 0.5% for visible energies larger than 2 MeV. The uncertainty in the cosmogenic Li9 and He8 background is reduced from 45% to 30% in the near detectors. A detailed investigation of the spent nuclear fuel history improves its uncertainty from 100% to 30%. Analysis of the relative ν¯e rates and energy spectra among detectors yields sin22θ13=0.0856±0.0029 and Δm322=(2.471−0.070+0.068)×10−3  eV2 assuming the normal hierarchy, and Δm322=−(2.575−0.070+0.068)×10−3  eV2 assuming the inverted hierarchy.