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<button class="button is-small is-link">Go</button> </div> </div> </form> </div> </div> <ol class="breathe-horizontal" start="1"> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2006.14982">arXiv:2006.14982</a> <span> [<a href="https://arxiv.org/pdf/2006.14982">pdf</a>, <a href="https://arxiv.org/format/2006.14982">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/10.1088/1748-0221/16/01/P01017">10.1088/1748-0221/16/01/P01017 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Performance of ALICE AD modules in the CERN PS test beam </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Broz%2C+M">M. Broz</a>, <a href="/search/physics?searchtype=author&query=Noris%2C+J+C+C">J. C. Cabanillas Noris</a>, <a href="/search/physics?searchtype=author&query=Villar%2C+E+C">E. Calvo Villar</a>, <a href="/search/physics?searchtype=author&query=Galvan%2C+C+D">C. Duarte Galvan</a>, <a href="/search/physics?searchtype=author&query=Endress%2C+E">E. Endress</a>, <a href="/search/physics?searchtype=author&query=Beltran%2C+L+G+E">L. G. Espinoza Beltran</a>, <a href="/search/physics?searchtype=author&query=Tellez%2C+A+F">A. Fernandez Tellez</a>, <a href="/search/physics?searchtype=author&query=Finogeev%2C+D">D. Finogeev</a>, <a href="/search/physics?searchtype=author&query=Gago%2C+A+M">A. M. Gago</a>, <a href="/search/physics?searchtype=author&query=Corral%2C+G+H">G. Herrera Corral</a>, <a href="/search/physics?searchtype=author&query=Kim%2C+T">T. Kim</a>, <a href="/search/physics?searchtype=author&query=Kurepin%2C+A">A. Kurepin</a>, <a href="/search/physics?searchtype=author&query=Kurepin%2C+A+B">A. B. Kurepin</a>, <a href="/search/physics?searchtype=author&query=Kurepin%2C+N">N. Kurepin</a>, <a href="/search/physics?searchtype=author&query=Monzon%2C+I+L">I. Leon Monzon</a>, <a href="/search/physics?searchtype=author&query=Hernandez%2C+M+I+M">M. I. Martinez Hernandez</a>, <a href="/search/physics?searchtype=author&query=Mayer%2C+C">C. Mayer</a>, <a href="/search/physics?searchtype=author&query=Mieskolainen%2C+M+M">M. M. Mieskolainen</a>, <a href="/search/physics?searchtype=author&query=Orava%2C+R">R. Orava</a>, <a href="/search/physics?searchtype=author&query=Moreno%2C+L+A+P">L. A. Perez Moreno</a>, <a href="/search/physics?searchtype=author&query=Revol%2C+J+-">J. -P. Revol</a>, <a href="/search/physics?searchtype=author&query=Cahuantzi%2C+M+R">M. Rodriguez Cahuantzi</a>, <a href="/search/physics?searchtype=author&query=Torres%2C+S+R">S. Rojas Torres</a>, <a href="/search/physics?searchtype=author&query=Serebryakov%2C+D">D. Serebryakov</a>, <a href="/search/physics?searchtype=author&query=Shabanov%2C+A">A. Shabanov</a> , et al. (2 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="2006.14982v1-abstract-short" style="display: inline;"> Two modules of the AD detector have been studied with the test beam at the T10 facility at CERN. The AD detector is made of scintillator pads read out by wave-length shifters (WLS)coupled to clean fibres that carry the produced light to photo-multiplier tubes (PMTs). In ALICE the AD is used to trigger and study the physics of diffractive and ultra-peripheral collisions as well as for a variety of… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2006.14982v1-abstract-full').style.display = 'inline'; document.getElementById('2006.14982v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2006.14982v1-abstract-full" style="display: none;"> Two modules of the AD detector have been studied with the test beam at the T10 facility at CERN. The AD detector is made of scintillator pads read out by wave-length shifters (WLS)coupled to clean fibres that carry the produced light to photo-multiplier tubes (PMTs). In ALICE the AD is used to trigger and study the physics of diffractive and ultra-peripheral collisions as well as for a variety of technical tasks like beam-gas background monitoring or as a luminometer. The position dependence of the modules' efficiency has been measured and the effect of hits on the WLS or PMTs has been evaluated. The charge deposited by pions and protons has been measured at different momenta of the test beam. The time resolution is determined as a function of the deposited charge. These results are important ingredients to better understand the AD detector, to benchmark the corresponding simulations, and very importantly they served as a baseline for a similar device, the Forward Diffractive Detector (FDD), being currently built and that will be in operation in ALICE during the LHC Runs 3 and 4. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2006.14982v1-abstract-full').style.display = 'none'; document.getElementById('2006.14982v1-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> 26 June, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2020. </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">12 pages, 9 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1709.02026">arXiv:1709.02026</a> <span> [<a href="https://arxiv.org/pdf/1709.02026">pdf</a>, <a href="https://arxiv.org/format/1709.02026">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="Nuclear Experiment">nucl-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/10.1016/j.nima.2017.12.042">10.1016/j.nima.2017.12.042 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Testing FLUKA on neutron activation of Si and Ge at nuclear research reactor using gamma spectroscopy </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Bazo%2C+J">Jose Bazo</a>, <a href="/search/physics?searchtype=author&query=Rojas%2C+J+M">Jairo M. Rojas</a>, <a href="/search/physics?searchtype=author&query=Best%2C+S">Sergio Best</a>, <a href="/search/physics?searchtype=author&query=Bruna%2C+R">Ruben Bruna</a>, <a href="/search/physics?searchtype=author&query=Endress%2C+E">Eric Endress</a>, <a href="/search/physics?searchtype=author&query=Mendoza%2C+P">Pablo Mendoza</a>, <a href="/search/physics?searchtype=author&query=Poma%2C+V">Victor Poma</a>, <a href="/search/physics?searchtype=author&query=Gago%2C+A+M">Alberto M. Gago</a> </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="1709.02026v2-abstract-short" style="display: inline;"> Samples of two characteristic semiconductor sensor materials, silicon and germanium, have been irradiated with neutrons produced at the RP-10 Nuclear Research Reactor at 4.5 MW. Their radionuclides photon spectra have been measured with high resolution gamma spectroscopy, quantifying four radioisotopes ($^{28}$Al, $^{29}$Al for Si and $^{75}$Ge and $^{77}$Ge for Ge). We have compared the radionucl… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1709.02026v2-abstract-full').style.display = 'inline'; document.getElementById('1709.02026v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1709.02026v2-abstract-full" style="display: none;"> Samples of two characteristic semiconductor sensor materials, silicon and germanium, have been irradiated with neutrons produced at the RP-10 Nuclear Research Reactor at 4.5 MW. Their radionuclides photon spectra have been measured with high resolution gamma spectroscopy, quantifying four radioisotopes ($^{28}$Al, $^{29}$Al for Si and $^{75}$Ge and $^{77}$Ge for Ge). We have compared the radionuclides production and their emission spectrum data with Monte Carlo simulation results from FLUKA. Thus we have tested FLUKA's low energy neutron library (ENDF/B-VIIR) and decay photon scoring with respect to the activation of these semiconductors. We conclude that FLUKA is capable of predicting relative photon peak amplitudes, with gamma intensities greater than 1%, of produced radionuclides with an average uncertainty of 13%. This work allows us to estimate the corresponding systematic error on neutron activation simulation studies of these sensor materials. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1709.02026v2-abstract-full').style.display = 'none'; document.getElementById('1709.02026v2-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> 20 December, 2017; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 6 September, 2017; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 2017. </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">18 pages, 5 figures; figure added, minor changes, typos corrected</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Nucl. Instr. Meth. Phys. Res., A 885 (2018) 1-6 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1607.00704">arXiv:1607.00704</a> <span> [<a href="https://arxiv.org/pdf/1607.00704">pdf</a>, <a href="https://arxiv.org/format/1607.00704">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.94.092005">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/1601.05471">arXiv:1601.05471</a> <span> [<a href="https://arxiv.org/pdf/1601.05471">pdf</a>, <a href="https://arxiv.org/format/1601.05471">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"> Long-Baseline Neutrino Facility (LBNF) and Deep Underground Neutrino Experiment (DUNE) Conceptual Design Report Volume 1: The LBNF and DUNE Projects </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Acciarri%2C+R">R. Acciarri</a>, <a href="/search/physics?searchtype=author&query=Acero%2C+M+A">M. A. Acero</a>, <a href="/search/physics?searchtype=author&query=Adamowski%2C+M">M. Adamowski</a>, <a href="/search/physics?searchtype=author&query=Adams%2C+C">C. Adams</a>, <a href="/search/physics?searchtype=author&query=Adamson%2C+P">P. Adamson</a>, <a href="/search/physics?searchtype=author&query=Adhikari%2C+S">S. Adhikari</a>, <a href="/search/physics?searchtype=author&query=Ahmad%2C+Z">Z. Ahmad</a>, <a href="/search/physics?searchtype=author&query=Albright%2C+C+H">C. H. Albright</a>, <a href="/search/physics?searchtype=author&query=Alion%2C+T">T. Alion</a>, <a href="/search/physics?searchtype=author&query=Amador%2C+E">E. Amador</a>, <a href="/search/physics?searchtype=author&query=Anderson%2C+J">J. Anderson</a>, <a href="/search/physics?searchtype=author&query=Anderson%2C+K">K. Anderson</a>, <a href="/search/physics?searchtype=author&query=Andreopoulos%2C+C">C. Andreopoulos</a>, <a href="/search/physics?searchtype=author&query=Andrews%2C+M">M. Andrews</a>, <a href="/search/physics?searchtype=author&query=Andrews%2C+R">R. Andrews</a>, <a href="/search/physics?searchtype=author&query=Anghel%2C+I">I. Anghel</a>, <a href="/search/physics?searchtype=author&query=Anjos%2C+J+d">J. d. Anjos</a>, <a href="/search/physics?searchtype=author&query=Ankowski%2C+A">A. Ankowski</a>, <a href="/search/physics?searchtype=author&query=Antonello%2C+M">M. Antonello</a>, <a href="/search/physics?searchtype=author&query=ArandaFernandez%2C+A">A. ArandaFernandez</a>, <a href="/search/physics?searchtype=author&query=Ariga%2C+A">A. Ariga</a>, <a href="/search/physics?searchtype=author&query=Ariga%2C+T">T. Ariga</a>, <a href="/search/physics?searchtype=author&query=Aristizabal%2C+D">D. Aristizabal</a>, <a href="/search/physics?searchtype=author&query=Arrieta-Diaz%2C+E">E. Arrieta-Diaz</a>, <a href="/search/physics?searchtype=author&query=Aryal%2C+K">K. Aryal</a> , et al. (780 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="1601.05471v1-abstract-short" style="display: inline;"> This document presents the Conceptual Design Report (CDR) put forward by an international neutrino community to pursue the Deep Underground Neutrino Experiment at the Long-Baseline Neutrino Facility (LBNF/DUNE), a groundbreaking science experiment for long-baseline neutrino oscillation studies and for neutrino astrophysics and nucleon decay searches. The DUNE far detector will be a very large modu… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1601.05471v1-abstract-full').style.display = 'inline'; document.getElementById('1601.05471v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1601.05471v1-abstract-full" style="display: none;"> This document presents the Conceptual Design Report (CDR) put forward by an international neutrino community to pursue the Deep Underground Neutrino Experiment at the Long-Baseline Neutrino Facility (LBNF/DUNE), a groundbreaking science experiment for long-baseline neutrino oscillation studies and for neutrino astrophysics and nucleon decay searches. The DUNE far detector will be a very large modular liquid argon time-projection chamber (LArTPC) located deep underground, coupled to the LBNF multi-megawatt wide-band neutrino beam. DUNE will also have a high-resolution and high-precision near detector. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1601.05471v1-abstract-full').style.display = 'none'; document.getElementById('1601.05471v1-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> 20 January, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2016. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1601.02984">arXiv:1601.02984</a> <span> [<a href="https://arxiv.org/pdf/1601.02984">pdf</a>, <a href="https://arxiv.org/format/1601.02984">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"> Long-Baseline Neutrino Facility (LBNF) and Deep Underground Neutrino Experiment (DUNE) Conceptual Design Report, Volume 4 The DUNE Detectors at LBNF </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Acciarri%2C+R">R. Acciarri</a>, <a href="/search/physics?searchtype=author&query=Acero%2C+M+A">M. A. Acero</a>, <a href="/search/physics?searchtype=author&query=Adamowski%2C+M">M. Adamowski</a>, <a href="/search/physics?searchtype=author&query=Adams%2C+C">C. Adams</a>, <a href="/search/physics?searchtype=author&query=Adamson%2C+P">P. Adamson</a>, <a href="/search/physics?searchtype=author&query=Adhikari%2C+S">S. Adhikari</a>, <a href="/search/physics?searchtype=author&query=Ahmad%2C+Z">Z. Ahmad</a>, <a href="/search/physics?searchtype=author&query=Albright%2C+C+H">C. H. Albright</a>, <a href="/search/physics?searchtype=author&query=Alion%2C+T">T. Alion</a>, <a href="/search/physics?searchtype=author&query=Amador%2C+E">E. Amador</a>, <a href="/search/physics?searchtype=author&query=Anderson%2C+J">J. Anderson</a>, <a href="/search/physics?searchtype=author&query=Anderson%2C+K">K. Anderson</a>, <a href="/search/physics?searchtype=author&query=Andreopoulos%2C+C">C. Andreopoulos</a>, <a href="/search/physics?searchtype=author&query=Andrews%2C+M">M. Andrews</a>, <a href="/search/physics?searchtype=author&query=Andrews%2C+R">R. Andrews</a>, <a href="/search/physics?searchtype=author&query=Anghel%2C+I">I. Anghel</a>, <a href="/search/physics?searchtype=author&query=Anjos%2C+J+d">J. d. Anjos</a>, <a href="/search/physics?searchtype=author&query=Ankowski%2C+A">A. Ankowski</a>, <a href="/search/physics?searchtype=author&query=Antonello%2C+M">M. Antonello</a>, <a href="/search/physics?searchtype=author&query=ArandaFernandez%2C+A">A. ArandaFernandez</a>, <a href="/search/physics?searchtype=author&query=Ariga%2C+A">A. Ariga</a>, <a href="/search/physics?searchtype=author&query=Ariga%2C+T">T. Ariga</a>, <a href="/search/physics?searchtype=author&query=Aristizabal%2C+D">D. Aristizabal</a>, <a href="/search/physics?searchtype=author&query=Arrieta-Diaz%2C+E">E. Arrieta-Diaz</a>, <a href="/search/physics?searchtype=author&query=Aryal%2C+K">K. Aryal</a> , et al. (779 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="1601.02984v1-abstract-short" style="display: inline;"> A description of the proposed detector(s) for DUNE at LBNF </span> <span class="abstract-full has-text-grey-dark mathjax" id="1601.02984v1-abstract-full" style="display: none;"> A description of the proposed detector(s) for DUNE at LBNF <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1601.02984v1-abstract-full').style.display = 'none'; document.getElementById('1601.02984v1-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> 12 January, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2016. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1512.06148">arXiv:1512.06148</a> <span> [<a href="https://arxiv.org/pdf/1512.06148">pdf</a>, <a href="https://arxiv.org/format/1512.06148">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"> Long-Baseline Neutrino Facility (LBNF) and Deep Underground Neutrino Experiment (DUNE) Conceptual Design Report Volume 2: The Physics Program for DUNE at LBNF </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=DUNE+Collaboration"> DUNE Collaboration</a>, <a href="/search/physics?searchtype=author&query=Acciarri%2C+R">R. Acciarri</a>, <a href="/search/physics?searchtype=author&query=Acero%2C+M+A">M. A. Acero</a>, <a href="/search/physics?searchtype=author&query=Adamowski%2C+M">M. Adamowski</a>, <a href="/search/physics?searchtype=author&query=Adams%2C+C">C. Adams</a>, <a href="/search/physics?searchtype=author&query=Adamson%2C+P">P. Adamson</a>, <a href="/search/physics?searchtype=author&query=Adhikari%2C+S">S. Adhikari</a>, <a href="/search/physics?searchtype=author&query=Ahmad%2C+Z">Z. Ahmad</a>, <a href="/search/physics?searchtype=author&query=Albright%2C+C+H">C. H. Albright</a>, <a href="/search/physics?searchtype=author&query=Alion%2C+T">T. Alion</a>, <a href="/search/physics?searchtype=author&query=Amador%2C+E">E. Amador</a>, <a href="/search/physics?searchtype=author&query=Anderson%2C+J">J. Anderson</a>, <a href="/search/physics?searchtype=author&query=Anderson%2C+K">K. Anderson</a>, <a href="/search/physics?searchtype=author&query=Andreopoulos%2C+C">C. Andreopoulos</a>, <a href="/search/physics?searchtype=author&query=Andrews%2C+M">M. Andrews</a>, <a href="/search/physics?searchtype=author&query=Andrews%2C+R">R. Andrews</a>, <a href="/search/physics?searchtype=author&query=Anghel%2C+I">I. Anghel</a>, <a href="/search/physics?searchtype=author&query=Anjos%2C+J+d">J. d. Anjos</a>, <a href="/search/physics?searchtype=author&query=Ankowski%2C+A">A. Ankowski</a>, <a href="/search/physics?searchtype=author&query=Antonello%2C+M">M. Antonello</a>, <a href="/search/physics?searchtype=author&query=ArandaFernandez%2C+A">A. ArandaFernandez</a>, <a href="/search/physics?searchtype=author&query=Ariga%2C+A">A. Ariga</a>, <a href="/search/physics?searchtype=author&query=Ariga%2C+T">T. Ariga</a>, <a href="/search/physics?searchtype=author&query=Aristizabal%2C+D">D. Aristizabal</a>, <a href="/search/physics?searchtype=author&query=Arrieta-Diaz%2C+E">E. Arrieta-Diaz</a> , et al. (780 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="1512.06148v2-abstract-short" style="display: inline;"> The Physics Program for the Deep Underground Neutrino Experiment (DUNE) at the Fermilab Long-Baseline Neutrino Facility (LBNF) is described. </span> <span class="abstract-full has-text-grey-dark mathjax" id="1512.06148v2-abstract-full" style="display: none;"> The Physics Program for the Deep Underground Neutrino Experiment (DUNE) at the Fermilab Long-Baseline Neutrino Facility (LBNF) is described. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1512.06148v2-abstract-full').style.display = 'none'; document.getElementById('1512.06148v2-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> 22 January, 2016; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 18 December, 2015; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2015. </p> </li> </ol> <div class="is-hidden-tablet">  <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">  <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 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