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is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevD.94.092005">10.1103/PhysRevD.94.092005 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Neutrino Flux Predictions for the NuMI Beam </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=MINERvA+Collaboration"> MINERvA Collaboration</a>, <a href="/search/physics?searchtype=author&query=Aliaga%2C+L">L. Aliaga</a>, <a href="/search/physics?searchtype=author&query=Kordosky%2C+M">M. Kordosky</a>, <a href="/search/physics?searchtype=author&query=Golan%2C+T">T. Golan</a>, <a href="/search/physics?searchtype=author&query=Altinok%2C+O">O. Altinok</a>, <a href="/search/physics?searchtype=author&query=Bellantoni%2C+L">L. Bellantoni</a>, <a href="/search/physics?searchtype=author&query=Bercellie%2C+A">A. Bercellie</a>, <a href="/search/physics?searchtype=author&query=Betancourt%2C+M">M. Betancourt</a>, <a href="/search/physics?searchtype=author&query=Bravar%2C+A">A. Bravar</a>, <a href="/search/physics?searchtype=author&query=Budd%2C+H">H. Budd</a>, <a href="/search/physics?searchtype=author&query=Carneiro%2C+M+F">M. F. Carneiro</a>, <a href="/search/physics?searchtype=author&query=Diaz%2C+G+A">G. A. Diaz</a>, <a href="/search/physics?searchtype=author&query=Endress%2C+E">E. Endress</a>, <a href="/search/physics?searchtype=author&query=Felix%2C+J">J. Felix</a>, <a href="/search/physics?searchtype=author&query=Fields%2C+L">L. Fields</a>, <a href="/search/physics?searchtype=author&query=Fine%2C+R">R. Fine</a>, <a href="/search/physics?searchtype=author&query=Gago%2C+A+M">A. M. Gago</a>, <a href="/search/physics?searchtype=author&query=Galindo%2C+R">R. Galindo</a>, <a href="/search/physics?searchtype=author&query=Gallagher%2C+H">H. Gallagher</a>, <a href="/search/physics?searchtype=author&query=Gran%2C+R">R. Gran</a>, <a href="/search/physics?searchtype=author&query=Harris%2C+D+A">D. A. Harris</a>, <a href="/search/physics?searchtype=author&query=Higuera%2C+A">A. Higuera</a>, <a href="/search/physics?searchtype=author&query=Hurtado%2C+K">K. Hurtado</a>, <a href="/search/physics?searchtype=author&query=Kiveni%2C+M">M. Kiveni</a>, <a href="/search/physics?searchtype=author&query=Kleykamp%2C+J">J. Kleykamp</a> , et al. (36 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1607.00704v3-abstract-short" style="display: inline;"> Knowledge of the neutrino flux produced by the Neutrinos at the Main Injector (NuMI) beamline is essential to the neutrino oscillation and neutrino interaction measurements of the MINERvA, MINOS+, NOvA and MicroBooNE experiments at Fermi National Accelerator Laboratory. We have produced a flux prediction which uses all available and relevant hadron production data, incorporating measurements of pa… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1607.00704v3-abstract-full').style.display = 'inline'; document.getElementById('1607.00704v3-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1607.00704v3-abstract-full" style="display: none;"> Knowledge of the neutrino flux produced by the Neutrinos at the Main Injector (NuMI) beamline is essential to the neutrino oscillation and neutrino interaction measurements of the MINERvA, MINOS+, NOvA and MicroBooNE experiments at Fermi National Accelerator Laboratory. We have produced a flux prediction which uses all available and relevant hadron production data, incorporating measurements of particle production off of thin targets as well as measurements of particle yields from a spare NuMI target exposed to a 120 GeV proton beam. The result is the most precise flux prediction achieved for a neutrino beam in the one to tens of GeV energy region. We have also compared the prediction to in situ measurements of the neutrino flux and find good agreement. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1607.00704v3-abstract-full').style.display = 'none'; document.getElementById('1607.00704v3-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 11 July, 2016; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 3 July, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2016. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">v2 includes supplemental material consisting of the flux prediction and uncertainties in ascii and root format, a program to read the ascii datafiles, and a short guide with additional details. v3 fixes a couple of typographical errors on the units for some quantities in the beam focusing section</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> Fermilab PUB-16-091-ND </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. D 94, 092005 (2016) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1604.03920">arXiv:1604.03920</a> <span> [<a href="https://arxiv.org/pdf/1604.03920">pdf</a>, <a href="https://arxiv.org/format/1604.03920">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevD.94.012002">10.1103/PhysRevD.94.012002 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Measurement of $K^{+}$ production in charged-current $谓_渭$ interactions </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Marshall%2C+C+M">C. M. Marshall</a>, <a href="/search/physics?searchtype=author&query=Aliaga%2C+L">L. Aliaga</a>, <a href="/search/physics?searchtype=author&query=Altinok%2C+O">O. Altinok</a>, <a href="/search/physics?searchtype=author&query=Bellantoni%2C+L">L. Bellantoni</a>, <a href="/search/physics?searchtype=author&query=Bercellie%2C+A">A. Bercellie</a>, <a href="/search/physics?searchtype=author&query=Betancourt%2C+M">M. Betancourt</a>, <a href="/search/physics?searchtype=author&query=Bodek%2C+A">A. Bodek</a>, <a href="/search/physics?searchtype=author&query=Bravar%2C+A">A. Bravar</a>, <a href="/search/physics?searchtype=author&query=Budd%2C+H">H. Budd</a>, <a href="/search/physics?searchtype=author&query=Cai%2C+T">T. Cai</a>, <a href="/search/physics?searchtype=author&query=Carneiro%2C+M+F">M. F. Carneiro</a>, <a href="/search/physics?searchtype=author&query=Chvojka%2C+J">J. Chvojka</a>, <a href="/search/physics?searchtype=author&query=da+Motta%2C+H">H. da Motta</a>, <a href="/search/physics?searchtype=author&query=Devan%2C+J">J. Devan</a>, <a href="/search/physics?searchtype=author&query=Dytman%2C+S+A">S. A. Dytman</a>, <a href="/search/physics?searchtype=author&query=D%C3%ADaz%2C+G+A">G. A. D铆az</a>, <a href="/search/physics?searchtype=author&query=Eberly%2C+B">B. Eberly</a>, <a href="/search/physics?searchtype=author&query=Endress%2C+E">E. Endress</a>, <a href="/search/physics?searchtype=author&query=Felix%2C+J">J. Felix</a>, <a href="/search/physics?searchtype=author&query=Fields%2C+L">L. Fields</a>, <a href="/search/physics?searchtype=author&query=Filkins%2C+A">A. Filkins</a>, <a href="/search/physics?searchtype=author&query=Fine%2C+R">R. Fine</a>, <a href="/search/physics?searchtype=author&query=Gago%2C+A+M">A. M. Gago</a>, <a href="/search/physics?searchtype=author&query=Galindo%2C+R">R. Galindo</a>, <a href="/search/physics?searchtype=author&query=Gallagher%2C+H">H. Gallagher</a> , et al. (57 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1604.03920v3-abstract-short" style="display: inline;"> Production of K^{+} mesons in charged-current 谓_渭 interactions on plastic scintillator (CH) is measured using MINERvA exposed to the low-energy NuMI beam at Fermilab. Timing information is used to isolate a sample of 885 charged-current events containing a stopping K^{+} which decays at rest. The differential cross section in K^{+} kinetic energy, d蟽/dT_{K}, is observed to be relatively flat betwe… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1604.03920v3-abstract-full').style.display = 'inline'; document.getElementById('1604.03920v3-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1604.03920v3-abstract-full" style="display: none;"> Production of K^{+} mesons in charged-current 谓_渭 interactions on plastic scintillator (CH) is measured using MINERvA exposed to the low-energy NuMI beam at Fermilab. Timing information is used to isolate a sample of 885 charged-current events containing a stopping K^{+} which decays at rest. The differential cross section in K^{+} kinetic energy, d蟽/dT_{K}, is observed to be relatively flat between 0 and 500 MeV. Its shape is in good agreement with the prediction by the \textsc{genie} neutrino event generator when final-state interactions are included, however the data rate is lower than the prediction by 15\%. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1604.03920v3-abstract-full').style.display = 'none'; document.getElementById('1604.03920v3-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 25 July, 2016; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 13 April, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2016. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">added ancillary files with cross-section, statistical uncertainty covariance matrix and systematic uncertainty covariance matrix decomposed into flux and non-flux components</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> FERMILAB PUB-16-109-ND </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. D 94, 012002 (2016) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1604.01728">arXiv:1604.01728</a> <span> [<a href="https://arxiv.org/pdf/1604.01728">pdf</a>, <a href="https://arxiv.org/format/1604.01728">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevLett.117.111801">10.1103/PhysRevLett.117.111801 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Evidence for neutral-current diffractive neutral pion production from hydrogen in neutrino interactions on hydrocarbon </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=MINERvA+Collaboration"> MINERvA Collaboration</a>, <a href="/search/physics?searchtype=author&query=Wolcott%2C+J">J. Wolcott</a>, <a href="/search/physics?searchtype=author&query=Aliaga%2C+L">L. Aliaga</a>, <a href="/search/physics?searchtype=author&query=Altinok%2C+O">O. Altinok</a>, <a href="/search/physics?searchtype=author&query=Bercellie%2C+A">A. Bercellie</a>, <a href="/search/physics?searchtype=author&query=Betancourt%2C+M">M. Betancourt</a>, <a href="/search/physics?searchtype=author&query=Bodek%2C+A">A. Bodek</a>, <a href="/search/physics?searchtype=author&query=Bravar%2C+A">A. Bravar</a>, <a href="/search/physics?searchtype=author&query=Budd%2C+H">H. Budd</a>, <a href="/search/physics?searchtype=author&query=Cai%2C+T">T. Cai</a>, <a href="/search/physics?searchtype=author&query=Carneiro%2C+M+F">M. F. Carneiro</a>, <a href="/search/physics?searchtype=author&query=Chvojka%2C+J">J. Chvojka</a>, <a href="/search/physics?searchtype=author&query=da+Motta%2C+H">H. da Motta</a>, <a href="/search/physics?searchtype=author&query=Devan%2C+J">J. Devan</a>, <a href="/search/physics?searchtype=author&query=Dytman%2C+S+A">S. A. Dytman</a>, <a href="/search/physics?searchtype=author&query=D%C3%ADaz%2C+G+A">G. A. D铆az</a>, <a href="/search/physics?searchtype=author&query=Eberly%2C+B">B. Eberly</a>, <a href="/search/physics?searchtype=author&query=Endress%2C+E">E. Endress</a>, <a href="/search/physics?searchtype=author&query=Felix%2C+J">J. Felix</a>, <a href="/search/physics?searchtype=author&query=Fields%2C+L">L. Fields</a>, <a href="/search/physics?searchtype=author&query=Fine%2C+R">R. Fine</a>, <a href="/search/physics?searchtype=author&query=Galindo%2C+R">R. Galindo</a>, <a href="/search/physics?searchtype=author&query=Gallagher%2C+H">H. Gallagher</a>, <a href="/search/physics?searchtype=author&query=Golan%2C+T">T. Golan</a>, <a href="/search/physics?searchtype=author&query=Gran%2C+R">R. Gran</a> , et al. (46 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1604.01728v5-abstract-short" style="display: inline;"> The MINERvA experiment observes an excess of events containing electromagnetic showers relative to the expectation from Monte Carlo simulations in neutral-current neutrino interactions with mean beam energy of 4.5 GeV on a hydrocarbon target. The excess is characterized and found to be consistent with neutral-current neutral pion production with a broad energy distribution peaking at 7 GeV and a t… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1604.01728v5-abstract-full').style.display = 'inline'; document.getElementById('1604.01728v5-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1604.01728v5-abstract-full" style="display: none;"> The MINERvA experiment observes an excess of events containing electromagnetic showers relative to the expectation from Monte Carlo simulations in neutral-current neutrino interactions with mean beam energy of 4.5 GeV on a hydrocarbon target. The excess is characterized and found to be consistent with neutral-current neutral pion production with a broad energy distribution peaking at 7 GeV and a total cross section of 0.26 +- 0.02 (stat) +- 0.08 (sys) x 10^{-39} cm^{2}. The angular distribution, electromagnetic shower energy, and spatial distribution of the energy depositions of the excess are consistent with expectations from neutrino neutral-current diffractive neutral pion production from hydrogen in the hydrocarbon target. These data comprise the first direct experimental observation and constraint for a reaction that poses an important background process in neutrino oscillation experiments searching for muon neutrino to electron neutrino oscillations. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1604.01728v5-abstract-full').style.display = 'none'; document.getElementById('1604.01728v5-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 28 July, 2016; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 6 April, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2016. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">15 pages, 7 figures; accepted by Phys. Rev. Lett</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> FERMILAB-PUB-16-108-ND </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. Lett. 117, 111801 (2016) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1512.07699">arXiv:1512.07699</a> <span> [<a href="https://arxiv.org/pdf/1512.07699">pdf</a>, <a href="https://arxiv.org/format/1512.07699">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevD.93.112007">10.1103/PhysRevD.93.112007 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Measurement of Neutrino Flux from Neutrino-Electron Elastic Scattering </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=MINERvA+Collaboration"> MINERvA Collaboration</a>, <a href="/search/physics?searchtype=author&query=Park%2C+J">J. Park</a>, <a href="/search/physics?searchtype=author&query=Aliaga%2C+L">L. Aliaga</a>, <a href="/search/physics?searchtype=author&query=Altinok%2C+O">O. Altinok</a>, <a href="/search/physics?searchtype=author&query=Bellantoni%2C+L">L. Bellantoni</a>, <a href="/search/physics?searchtype=author&query=Bercellie%2C+A">A. Bercellie</a>, <a href="/search/physics?searchtype=author&query=Betancourt%2C+M">M. Betancourt</a>, <a href="/search/physics?searchtype=author&query=Bodek%2C+A">A. Bodek</a>, <a href="/search/physics?searchtype=author&query=Bravar%2C+A">A. Bravar</a>, <a href="/search/physics?searchtype=author&query=Budd%2C+H">H. Budd</a>, <a href="/search/physics?searchtype=author&query=Cai%2C+T">T. Cai</a>, <a href="/search/physics?searchtype=author&query=Carneiro%2C+M+F">M. F. Carneiro</a>, <a href="/search/physics?searchtype=author&query=Christy%2C+M+E">M. E. Christy</a>, <a href="/search/physics?searchtype=author&query=Chvojka%2C+J">J. Chvojka</a>, <a href="/search/physics?searchtype=author&query=da+Motta%2C+H">H. da Motta</a>, <a href="/search/physics?searchtype=author&query=Dytman%2C+S+A">S. A. Dytman</a>, <a href="/search/physics?searchtype=author&query=Diaz%2C+G+A">G. A. Diaz</a>, <a href="/search/physics?searchtype=author&query=Eberly%2C+B">B. Eberly</a>, <a href="/search/physics?searchtype=author&query=Felix%2C+J">J. Felix</a>, <a href="/search/physics?searchtype=author&query=Fields%2C+L">L. Fields</a>, <a href="/search/physics?searchtype=author&query=Fine%2C+R">R. Fine</a>, <a href="/search/physics?searchtype=author&query=Gago%2C+A+M">A. M. Gago</a>, <a href="/search/physics?searchtype=author&query=Galindo%2C+R">R. Galindo</a>, <a href="/search/physics?searchtype=author&query=Ghosh%2C+A">A. Ghosh</a>, <a href="/search/physics?searchtype=author&query=Golan%2C+T">T. Golan</a> , et al. (44 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1512.07699v3-abstract-short" style="display: inline;"> Muon-neutrino elastic scattering on electrons is an observable neutrino process whose cross section is precisely known. Consequently a measurement of this process in an accelerator-based $谓_渭$ beam can improve the knowledge of the absolute neutrino flux impinging upon the detector; typically this knowledge is limited to $\sim$ 10% due to uncertainties in hadron production and focusing. We have iso… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1512.07699v3-abstract-full').style.display = 'inline'; document.getElementById('1512.07699v3-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1512.07699v3-abstract-full" style="display: none;"> Muon-neutrino elastic scattering on electrons is an observable neutrino process whose cross section is precisely known. Consequently a measurement of this process in an accelerator-based $谓_渭$ beam can improve the knowledge of the absolute neutrino flux impinging upon the detector; typically this knowledge is limited to $\sim$ 10% due to uncertainties in hadron production and focusing. We have isolated a sample of 135 $\pm$ 17 neutrino-electron elastic scattering candidates in the segmented scintillator detector of MINERvA, after subtracting backgrounds and correcting for efficiency. We show how this sample can be used to reduce the total uncertainty on the NuMI $谓_渭$ flux from 9% to 6%. Our measurement provides a flux constraint that is useful to other experiments using the NuMI beam, and this technique is applicable to future neutrino beams operating at multi-GeV energies. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1512.07699v3-abstract-full').style.display = 'none'; document.getElementById('1512.07699v3-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 15 June, 2016; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 23 December, 2015; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2015. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">11 pages, 11 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> FERMILAB-PUB-15-575-ND </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. D 93, 112007 (2016) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1501.06431">arXiv:1501.06431</a> <span> [<a href="https://arxiv.org/pdf/1501.06431">pdf</a>, <a href="https://arxiv.org/format/1501.06431">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> </div> <p class="title is-5 mathjax"> MINERvA neutrino detector response measured with test beam data </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=MINERvA+Collaboration"> MINERvA Collaboration</a>, <a href="/search/physics?searchtype=author&query=Aliaga%2C+L">L. Aliaga</a>, <a href="/search/physics?searchtype=author&query=Altinok%2C+O">O. Altinok</a>, <a href="/search/physics?searchtype=author&query=Del+Castillo%2C+C+A">C. Araujo Del Castillo</a>, <a href="/search/physics?searchtype=author&query=Bagby%2C+L">L. Bagby</a>, <a href="/search/physics?searchtype=author&query=Bellantoni%2C+L">L. Bellantoni</a>, <a href="/search/physics?searchtype=author&query=Bergan%2C+W+F">W. F. Bergan</a>, <a href="/search/physics?searchtype=author&query=Bodek%2C+A">A. Bodek</a>, <a href="/search/physics?searchtype=author&query=Bradford%2C+R">R. Bradford</a>, <a href="/search/physics?searchtype=author&query=Bravar%2C+A">A. Bravar</a>, <a href="/search/physics?searchtype=author&query=Budd%2C+H">H. Budd</a>, <a href="/search/physics?searchtype=author&query=Butkevich%2C+A">A. Butkevich</a>, <a href="/search/physics?searchtype=author&query=Caicedo%2C+D+A+M">D. A. Martinez Caicedo</a>, <a href="/search/physics?searchtype=author&query=Carneiro%2C+M+F">M. F. Carneiro</a>, <a href="/search/physics?searchtype=author&query=Christy%2C+M+E">M. E. Christy</a>, <a href="/search/physics?searchtype=author&query=Chvojka%2C+J">J. Chvojka</a>, <a href="/search/physics?searchtype=author&query=da+Motta%2C+H">H. da Motta</a>, <a href="/search/physics?searchtype=author&query=Devan%2C+J">J. Devan</a>, <a href="/search/physics?searchtype=author&query=Diaz%2C+G+A">G. A. Diaz</a>, <a href="/search/physics?searchtype=author&query=Dytman%2C+S+A">S. A. Dytman</a>, <a href="/search/physics?searchtype=author&query=Eberly%2C+B">B. Eberly</a>, <a href="/search/physics?searchtype=author&query=Felix%2C+J">J. Felix</a>, <a href="/search/physics?searchtype=author&query=Fields%2C+L">L. Fields</a>, <a href="/search/physics?searchtype=author&query=Fine%2C+R">R. Fine</a>, <a href="/search/physics?searchtype=author&query=Flight%2C+R">R. Flight</a> , et al. (63 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1501.06431v2-abstract-short" style="display: inline;"> The MINERvA collaboration operated a scaled-down replica of the solid scintillator tracking and sampling calorimeter regions of the MINERvA detector in a hadron test beam at the Fermilab Test Beam Facility. This article reports measurements with samples of protons, pions, and electrons from 0.35 to 2.0 GeV/c momentum. The calorimetric response to protons, pions, and electrons are obtained from the… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1501.06431v2-abstract-full').style.display = 'inline'; document.getElementById('1501.06431v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1501.06431v2-abstract-full" style="display: none;"> The MINERvA collaboration operated a scaled-down replica of the solid scintillator tracking and sampling calorimeter regions of the MINERvA detector in a hadron test beam at the Fermilab Test Beam Facility. This article reports measurements with samples of protons, pions, and electrons from 0.35 to 2.0 GeV/c momentum. The calorimetric response to protons, pions, and electrons are obtained from these data. A measurement of the parameter in Birks' law and an estimate of the tracking efficiency are extracted from the proton sample. Overall the data are well described by a Geant4-based Monte Carlo simulation of the detector and particle interactions with agreements better than 4%, though some features of the data are not precisely modeled. These measurements are used to tune the MINERvA detector simulation and evaluate systematic uncertainties in support of the MINERvA neutrino cross section measurement program. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1501.06431v2-abstract-full').style.display = 'none'; document.getElementById('1501.06431v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 7 April, 2015; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 26 January, 2015; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2015. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">as accepted by NIM A</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> FERMILAB-PUB-15-018-ND </p> </li> </ol> <div class="is-hidden-tablet"> <!-- feedback for mobile only --> <span class="help" style="display: inline-block;"><a href="https://github.com/arXiv/arxiv-search/releases">Search v0.5.6 released 2020-02-24</a> </span> </div> </div> </main> <footer> <div class="columns is-desktop" role="navigation" aria-label="Secondary"> <!-- MetaColumn 1 --> <div class="column"> <div class="columns"> <div class="column"> <ul class="nav-spaced"> <li><a href="https://info.arxiv.org/about">About</a></li> <li><a href="https://info.arxiv.org/help">Help</a></li> </ul> </div> <div class="column"> <ul class="nav-spaced"> <li> <svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512" class="icon filter-black" role="presentation"><title>contact arXiv</title><desc>Click here to contact arXiv</desc><path d="M502.3 190.8c3.9-3.1 9.7-.2 9.7 4.7V400c0 26.5-21.5 48-48 48H48c-26.5 0-48-21.5-48-48V195.6c0-5 5.7-7.8 9.7-4.7 22.4 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