Supernova neutrino detection in NOvA,Journal of Cosmology and Astroparticle Physics

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Supernova neutrino detection in NOvA
Journal of Cosmology and Astroparticle Physics ( IF 5.3 ) Pub Date : 2020-10-05 , DOI: 10.1088/1475-7516/2020/10/014
M.A. Acero ₁ , P. Adamson ₂ , G. Agam ₃ , L. Aliaga ₂ , T. Alion ₄ , V. Allakhverdian ₅ , N. Anfimov ₅ , A. Antoshkin ₅ , E. Arrieta-Diaz ₆ , L. Asquith ₄ , A. Aurisano ₇ , A. Back ₈ , C. Backhouse _{9,

10} , M. Baird _{4,

11,

12} , N. Balashov ₅ , P. Baldi ₁₃ , B.A. Bambah ₁₄ , S. Bashar ₁₅ , K. Bays _{3,

9} , S. Bending ₁₀ , R. Bernstein ₂ , V. Bhatnagar ₁₆ , B. Bhuyan ₁₇ , J. Bian _{13,

18} , J. Blair ₁₉ , A.C. Booth ₄ , P. Bour ₂₀ , R. Bowles ₁₁ , C. Bromberg ₂₁ , N. Buchanan ₂₂ , A. Butkevich ₂₃ , V. Bychkov ₁₈ , S. Calvez ₂₂ , T.J. Carroll _{24,

25} , E. Catano-Mur _{8,

26} , S. Childress ₂ , B.C. Choudhary ₂₇ , T. E. Coan ₂₈ , M. Colo ₂₆ , L. Corwin ₂₉ , L. Cremonesi ₁₀ , G.S. Davies _{11,

30} , P.F. Derwent ₂ , P. Ding ₂ , Z. Djurcic ₃₁ , M. Dolce ₁₅ , D. Doyle ₂₂ , D. Dueñas Tonguino ₇ , E.C. Dukes ₁₂ , P. Dung ₂₄ , H. Duyang ₃₂ , S. Edayath ₃₃ , R. Ehrlich ₁₂ , M. Elkins ₈ , G.J. Feldman ₃₄ , P. Filip ₃₅ , W. Flanagan ₃₆ , J. Franc ₂₀ , M.J. Frank ₃₇ , H.R. Gallagher ₁₅ , R. Gandrajula ₂₁ , F. Gao ₃₈ , S. Germani ₁₀ , A. Giri ₃₉ , R.A. Gomes ₄₀ , M.C. Goodman ₃₁ , V. Grichine ₄₁ , M. Groh ₁₁ , R. Group ₁₂ , B. Guo ₃₂ , A. Habig ₄₂ , F. Hakl ₄₃ , A. Hall ₁₂ , J. Hartnell ₄ , R. Hatcher ₂ , A. Hatzikoutelis ₄₄ , K. Heller ₁₈ , J. Hewes ₇ , A. Himmel ₂ , A. Holin ₁₀ , B. Howard ₁₁ , J. Huang ₂₄ , J. Hylen ₂ , F. Jediny ₂₀ , C. Johnson ₂₂ , M. Judah ₂₂ , I. Kakorin ₅ , D. Kalra ₁₆ , D. M. Kaplan ₃ , R. Keloth ₃₃ , O. Klimov ₅ , L.W. Koerner ₁₉ , L. Kolupaeva ₅ , S. Kotelnikov ₄₁ , M. Kubu ₂₀ , Ch. Kullenberg ₅ , A. Kumar ₁₆ , C.D. Kuruppu ₃₂ , V. Kus ₂₀ , T. Lackey ₁₁ , K. Lang ₂₄ , L. Li ₁₃ , S. Lin ₂₂ , A. Lister ₂₅ , M. Lokajicek ₃₅ , S. Luchuk ₂₃ , S. Magill ₃₁ , W.A. Mann ₁₅ , M.L. Marshak ₁₈ , M. Martinez-Casales ₈ , V. Matveev ₂₃ , B. Mayes ₄ , D.P. Méndez ₄ , M.D. Messier ₁₁ , H. Meyer ₄₅ , T. Miao ₂ , W.H. Miller ₁₈ , S.R. Mishra ₃₂ , A. Mislivec ₁₈ , R. Mohanta ₁₄ , A. Moren ₄₂ , A. Morozova ₅ , L. Mualem ₉ , M. Muether ₄₅ , S. Mufson ₁₁ , K. Mulder ₁₀ , R. Murphy ₁₁ , J. Musser ₁₁ , D. Naples ₃₈ , N. Nayak ₁₃ , J.K. Nelson ₂₆ , R. Nichol ₁₀ , G. Nikseresht ₃ , E. Niner _{2,

11} , A. Norman ₂ , A. Norrick ₂ , T. Nosek ₄₆ , A. Olshevskiy ₅ , T. Olson ₁₅ , J. Paley ₂ , R.B. Patterson ₉ , G. Pawloski ₁₈ , O. Petrova ₅ , R. Petti ₃₂ , R.K. Plunkett ₂ , F. Psihas _{11,

24} , A. Rafique ₃₁ , V. Raj ₉ , B. Ramson ₂ , B. Rebel _{2,

25} , P. Rojas ₂₂ , V. Ryabov ₄₁ , O. Samoylov ₅ , M.C. Sanchez _{8,

31} , S. Sánchez Falero ₈ , I. S. Seong ₁₃ , P. Shanahan ₂ , A. Sheshukov ₅ , P. Singh ₂₇ , V. Singh ₄₇ , E. Smith ₁₁ , J. Smolik ₂₀ , P. Snopok ₃ , N. Solomey ₄₅ , A. Sousa ₇ , K. Soustruznik ₄₆ , M. Strait ₁₈ , L. Suter _{2,

31} , A. Sutton ₁₂ , C. Sweeney ₁₀ , R. L. Talaga ₃₁ , B. Tapia Oregui ₂₄ , P. Tas ₄₆ , R.B. Thayyullathil ₃₃ , J. Thomas _{10,

25} , E. Tiras ₈ , D. Torbunov ₁₈ , J. Tripathi ₁₆ , A. Tsaris ₂ , Y. Torun ₃ , J. Urheim ₁₁ , P. Vahle ₂₆ , Z. Vallari ₉ , J. Vasel ₁₁ , P. Vokac ₂₀ , T. Vrba ₂₀ , M. Wallbank ₇ , T. K. Warburton ₈ , M. Wetstein ₈ , D. Whittington _{11,

48} , D.A. Wickremasinghe ₂ , S.G. Wojcicki ₄₉ , J. Wolcott ₁₅ , A. Yallappa Dombara ₄₈ , K. Yonehara ₂ , S. Yu _{3,

31} , Y. Yu ₃ , S. Zadorozhnyy ₂₃ , J. Zalesak ₃₅ , Y. Zhang ₄ , R. Zwaska ₂

Affiliation

Universidad del Atlantico, Carrera 30 No. 8-49, Puerto Colombia, Atlantico, Colombia
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, U.S.A.
Illinois Institute of Technology, Chicago IL 60616, U.S.A.
Department of Physics and Astronomy, University of Sussex, Falmer, Brighton BN1 9QH, United Kingdom
Joint Institute for Nuclear Research, Dubna, Moscow region 141980, Russia
Universidad del Magdalena, Carrera 32 No 22–08 Santa Marta, Colombia
Department of Physics, University of Cincinnati, Cincinnati, Ohio 45221, U.S.A.
Department of Physics and Astronomy, Iowa State University, Ames, Iowa 50011, U.S.A.
California Institute of Technology, Pasadena, California 91125, U.S.A.
Physics and Astronomy Dept., University College London, Gower Street, London WC1E 6BT, United Kingdom
Indiana University, Bloomington, Indiana 47405, U.S.A.
Department of Physics, University of Virginia, Charlottesville, Virginia 22904, U.S.A.
Department of Physics and Astronomy, University of California at Irvine, Irvine, California 92697, U.S.A.
School of Physics, University of Hyderabad, Hyderabad, 500 046, India
Department of Physics and Astronomy, Tufts University, Medford, Massachusetts 02155, U.S.A.
Department of Physics, Panjab University, Chandigarh, 160 014, India
Department of Physics, IIT Guwahati, Guwahati, 781 039, India
School of Physics and Astronomy, University of Minnesota Twin Cities, Minneapolis, Minnesota 55455, U.S.A.
Department of Physics, University of Houston, Houston, Texas 77204, U.S.A.
Czech Technical University in Prague, Brehova 7, 115 19 Prague 1, Czech Republic
Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, U.S.A.
Department of Physics, Colorado State University, Fort Collins, CO 80523-1875, U.S.A.
Institute for Nuclear Research of Russia, Academy of Sciences 7a, 60th October Anniversary prospect, Moscow 117312, Russia
Department of Physics, University of Texas at Austin, Austin, Texas 78712, U.S.A.
Department of Physics, University of Wisconsin-Madison, Madison, Wisconsin 53706, U.S.A.
Department of Physics, William & Mary, Williamsburg, Virginia 23187, U.S.A.
Department of Physics and Astrophysics, University of Delhi, Delhi 110007, India
Department of Physics, Southern Methodist University, Dallas, Texas 75275, U.S.A.
South Dakota School of Mines and Technology, Rapid City, South Dakota 57701, U.S.A.
University of Mississippi, University, Mississippi 38677, U.S.A.
Argonne National Laboratory, Argonne, Illinois 60439, U.S.A.
Department of Physics and Astronomy, University of South Carolina, Columbia, South Carolina 29208, U.S.A.
Department of Physics, Cochin University of Science and Technology, Kochi 682 022, India
Department of Physics, Harvard University, Cambridge, Massachusetts 02138, U.S.A.
Institute of Physics, The Czech Academy of Sciences, 182 21 Prague, Czech Republic
University of Dallas, 1845 E Northgate Drive, Irving, Texas 75062 U.S.A.
Department of Physics, University of South Alabama, Mobile, Alabama 36688, U.S.A.
Department of Physics, University of Pittsburgh, Pittsburgh, Pennsylvania 15260, U.S.A.
Department of Physics, IIT Hyderabad, Hyderabad, 502 205, India
Instituto de Física, Universidade Federal de Goiás, Goiânia, Goiás, 74690-900, Brazil
Nuclear Physics and Astrophysics Division, Lebedev Physical Institute, Leninsky Prospect 53, 119991 Moscow, Russia
Department of Physics and Astronomy, University of Minnesota Duluth, Duluth, Minnesota 55812, U.S.A.
Institute of Computer Science, The Czech Academy of Sciences, 182 07 Prague, Czech Republic
Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, U.S.A.
Department of Mathematics, Statistics, and Physics, Wichita State University, Wichita, Kansas 67206, U.S.A.
Charles University, Faculty of Mathematics and Physics, Institute of Particle and Nuclear Physics, Prague, Czech Republic
Department of Physics, Institute of Science, Banaras Hindu University, Varanasi, 221 005, India
Department of Physics, Syracuse University, Syracuse NY 13210, U.S.A.
Department of Physics, Stanford University, Stanford, California 94305, U.S.A.

The NOvA long-baseline neutrino experiment uses a pair of large, segmented, liquid-scintillator calorimeters to study neutrino oscillations, using GeV-scale neutrinos from the Fermilab NuMI beam. These detectors are also sensitive to the flux of neutrinos which are emitted during a core-collapse supernova through inverse beta decay interactions on carbon at energies of $\mathcal{O}(10~\text{MeV})$. This signature provides a means to study the dominant mode of energy release for a core-collapse supernova occurring in our galaxy. We describe the data-driven software trigger system developed and employed by the NOvA experiment to identify and record neutrino data from nearby galactic supernovae. This technique has been used by NOvA to self-trigger on potential core-collapse supernovae in our galaxy, with an estimated sensitivity reaching out to 10~kpc distance while achieving a detection efficiency of 23\% to 49\% for supernovae from progenitor stars with masses of 9.6M$_\odot$ to 27M$_\odot$, respectively.

中文翻译：

NOvA中的超新星中微子探测

NOvA 长基线中微子实验使用一对大型分段液体闪烁量热计来研究中微子振荡，使用来自费米实验室 NuMI 光束的 GeV 尺度中微子。这些探测器还对核心坍缩超新星期间通过碳上的逆β衰变相互作用以$\mathcal{O}(10~\text{MeV})$ 的能量发射的中微子通量敏感。这一特征为研究发生在我们银河系中的核心坍缩超新星的主要能量释放模式提供了一种手段。我们描述了由 NOvA 实验开发和使用的数据驱动软件触发系统，用于识别和记录来自附近星系超新星的中微子数据。这种技术已被 NOvA 用于自触发我们银河系中潜在的核心坍缩超新星，

更新日期：2020-10-05

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