Constraints on neutrino emission from nearby galaxies using the 2MASS redshift survey and IceCube,Journal of Cosmology and Astroparticle Physics

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Constraints on neutrino emission from nearby galaxies using the 2MASS redshift survey and IceCube
Journal of Cosmology and Astroparticle Physics ( IF 6.4 ) Pub Date : 2020-07-16 , DOI: 10.1088/1475-7516/2020/07/042
M.G. Aartsen ₁ , M. Ackermann ₂ , J. Adams ₁ , J.A. Aguilar ₃ , M. Ahlers ₄ , M. Ahrens ₅ , C. Alispach ₆ , K. Andeen ₇ , T. Anderson ₈ , I. Ansseau ₃ , G. Anton ₉ , C. Argüelles ₁₀ , J. Auffenberg ₁₁ , S. Axani ₁₀ , P. Backes ₁₁ , H. Bagherpour ₁ , X. Bai ₁₂ , A. Balagopal V. ₁₃ , A. Barbano ₆ , S.W. Barwick ₁₄ , B. Bastian ₂ , V. Baum ₁₅ , S. Baur ₃ , R. Bay ₁₆ , J.J. Beatty _{17,

18} , K.-H. Becker ₁₉ , J. Becker Tjus ₂₀ , S. BenZvi ₂₁ , D. Berley ₂₂ , E. Bernardini _{2,

23} , D.Z. Besson _{24,

25} , G. Binder _{16,

26} , D. Bindig ₁₉ , E. Blaufuss ₂₂ , S. Blot ₂ , C. Bohm ₅ , S. Böser ₁₅ , O. Botner ₂₇ , J. Böttcher ₁₁ , E. Bourbeau ₄ , J. Bourbeau ₂₈ , F. Bradascio ₂ , J. Braun ₂₈ , S. Bron ₆ , J. Brostean-Kaiser ₂ , A. Burgman ₂₇ , J. Buscher ₁₁ , R.S. Busse ₂₉ , T. Carver ₆ , C. Chen ₃₀ , E. Cheung ₂₂ , D. Chirkin ₂₈ , S. Choi ₃₁ , K. Clark ₃₂ , L. Classen ₂₉ , A. Coleman ₃₃ , G.H. Collin ₁₀ , J.M. Conrad ₁₀ , P. Coppin ₃₄ , P. Correa ₃₄ , D.F. Cowen _{8,

35} , R. Cross ₂₁ , P. Dave ₃₀ , C. De Clercq ₃₄ , J.J. DeLaunay ₈ , H. Dembinski ₃₃ , K. Deoskar ₅ , S. De Ridder ₃₆ , P. Desiati ₂₈ , K.D. de Vries ₃₄ , G. de Wasseige ₃₄ , M. de With ₃₇ , T. DeYoung ₃₈ , A. Diaz ₁₀ , J.C. Díaz-Vélez ₂₈ , H. Dujmovic ₁₃ , M. Dunkman ₈ , E. Dvorak ₁₂ , B. Eberhardt ₂₈ , T. Ehrhardt ₁₅ , P. Eller ₈ , R. Engel ₁₃ , P.A. Evenson ₃₃ , S. Fahey ₂₈ , A.R. Fazely ₃₉ , J. Felde ₂₂ , K. Filimonov ₁₆ , C. Finley ₅ , D. Fox ₃₅ , A. Franckowiak ₂ , E. Friedman ₂₂ , A. Fritz ₁₅ , T.K. Gaisser ₃₃ , J. Gallagher ₄₀ , E. Ganster ₁₁ , S. Garrappa ₂ , L. Gerhardt ₂₆ , K. Ghorbani ₂₈ , T. Glauch ₄₁ , T. Glüsenkamp ₉ , A. Goldschmidt ₂₆ , J.G. Gonzalez ₃₃ , D. Grant ₃₈ , Z. Griffith ₂₈ , S. Griswold ₂₁ , M. Günder ₁₁ , M. Gündüz ₂₀ , C. Haack ₁₁ , A. Hallgren ₂₇ , R. Halliday ₃₈ , L. Halve ₁₁ , F. Halzen ₂₈ , K. Hanson ₂₈ , A. Haungs ₁₃ , D. Hebecker ₃₇ , D. Heereman ₃ , P. Heix ₁₁ , K. Helbing ₁₉ , R. Hellauer ₂₂ , F. Henningsen ₄₁ , S. Hickford ₁₉ , J. Hignight ₄₂ , G.C. Hill ₄₃ , K.D. Hoffman ₂₂ , R. Hoffmann ₁₉ , T. Hoinka ₄₄ , B. Hokanson-Fasig ₂₈ , K. Hoshina _{28,

45} , F. Huang ₈ , M. Huber ₄₁ , T. Huber _{2,

13} , K. Hultqvist ₅ , M. Hünnefeld ₄₄ , R. Hussain ₂₈ , S. In ₃₁ , N. Iovine ₃ , A. Ishihara ₄₆ , G.S. Japaridze ₄₇ , M. Jeong ₃₁ , K. Jero ₂₈ , B.J.P. Jones ₄₈ , F. Jonske ₁₁ , R. Joppe ₁₁ , D. Kang ₁₃ , W. Kang ₃₁ , A. Kappes ₂₉ , D. Kappesser ₁₅ , T. Karg ₂ , M. Karl ₄₁ , A. Karle ₂₈ , U. Katz ₉ , M. Kauer ₂₈ , J.L. Kelley ₂₈ , A. Kheirandish ₂₈ , J. Kim ₃₁ , T. Kintscher ₂ , J. Kiryluk ₄₉ , T. Kittler ₉ , S.R. Klein _{16,

26} , R. Koirala ₃₃ , H. Kolanoski ₃₇ , L. Köpke ₁₅ , C. Kopper ₃₈ , S. Kopper ₅₀ , D.J. Koskinen ₄ , M. Kowalski _{2,

37} , K. Krings ₄₁ , G. Krückl ₁₅ , N. Kulacz ₄₂ , N. Kurahashi ₅₁ , A. Kyriacou ₄₃ , J.L. Lanfranchi ₈ , M.J. Larson ₂₂ , F. Lauber ₁₉ , J.P. Lazar ₂₈ , K. Leonard ₂₈ , A. Leszczyńska ₁₃ , M. Leuermann ₁₁ , Q.R. Liu ₂₈ , E. Lohfink ₁₅ , C.J. Lozano Mariscal ₂₉ , L. Lu ₄₆ , F. Lucarelli ₆ , J. Lünemann ₃₄ , W. Luszczak ₂₈ , Y. Lyu _{16,

26} , W.Y. Ma ₂ , J. Madsen ₅₂ , G. Maggi ₃₄ , K.B.M. Mahn ₃₈ , Y. Makino ₄₆ , P. Mallik ₁₁ , K. Mallot ₂₈ , S. Mancina ₂₈ , I.C. Mari{\c s} ₃ , R. Maruyama ₅₃ , K. Mase ₄₆ , R. Maunu ₂₂ , F. McNally ₅₄ , K. Meagher ₂₈ , M. Medici ₄ , A. Medina ₁₈ , M. Meier ₄₄ , S. Meighen-Berger ₄₁ , G. Merino ₂₈ , T. Meures ₃ , J. Micallef ₃₈ , D. Mockler ₃ , G. Momenté ₁₅ , T. Montaruli ₆ , R.W. Moore ₄₂ , R. Morse ₂₈ , M. Moulai ₁₀ , P. Muth ₁₁ , R. Nagai ₄₆ , U. Naumann ₁₉ , G. Neer ₃₈ , H. Niederhausen ₄₁ , M.U. Nisa ₃₈ , S.C. Nowicki ₃₈ , D.R. Nygren ₂₆ , A. Obertacke Pollmann ₁₉ , M. Oehler ₁₃ , A. Olivas ₂₂ , A. O'Murchadha ₃ , E. O'Sullivan ₅ , T. Palczewski _{16,

26} , H. Pandya ₃₃ , D.V. Pankova ₈ , N. Park ₂₈ , P. Peiffer ₁₅ , C. Pérez de los Heros ₂₇ , S. Philippen ₁₁ , D. Pieloth ₄₄ , E. Pinat ₃ , A. Pizzuto ₂₈ , M. Plum ₇ , A. Porcelli ₃₆ , P.B. Price ₁₆ , G.T. Przybylski ₂₆ , C. Raab ₃ , A. Raissi ₁ , M. Rameez ₄ , L. Rauch ₂ , K. Rawlins ₅₅ , I.C. Rea ₄₁ , R. Reimann ₁₁ , B. Relethford ₅₁ , M. Renschler ₁₃ , G. Renzi ₃ , E. Resconi ₄₁ , W. Rhode ₄₄ , M. Richman ₅₁ , S. Robertson ₂₆ , M. Rongen ₁₁ , C. Rott ₃₁ , T. Ruhe ₄₄ , D. Ryckbosch ₃₆ , D. Rysewyk ₃₈ , I. Safa ₂₈ , S.E. Sanchez Herrera ₃₈ , A. Sandrock ₄₄ , J. Sandroos ₁₅ , M. Santander ₅₀ , S. Sarkar ₅₆ , S. Sarkar ₄₂ , K. Satalecka ₂ , M. Schaufel ₁₁ , H. Schieler ₁₃ , P. Schlunder ₄₄ , T. Schmidt ₂₂ , A. Schneider ₂₈ , J. Schneider ₉ , F.G. Schröder _{13,

33} , L. Schumacher ₁₁ , S. Sclafani ₅₁ , D. Seckel ₃₃ , S. Seunarine ₅₂ , S. Shefali ₁₁ , M. Silva ₂₈ , R. Snihur ₂₈ , J. Soedingrekso ₄₄ , D. Soldin ₃₃ , M. Song ₂₂ , G.M. Spiczak ₅₂ , C. Spiering ₂ , J. Stachurska ₂ , M. Stamatikos ₁₈ , T. Stanev ₃₃ , R. Stein ₂ , J. Stettner ₁₁ , A. Steuer ₁₅ , T. Stezelberger ₂₆ , R.G. Stokstad ₂₆ , A. Stößl ₄₆ , N.L. Strotjohann ₂ , T. Stürwald ₁₁ , T. Stuttard ₄ , G.W. Sullivan ₂₂ , I. Taboada ₃₀ , F. Tenholt ₂₀ , S. Ter-Antonyan ₃₉ , A. Terliuk ₂ , S. Tilav ₃₃ , K. Tollefson ₃₈ , L. Tomankova ₂₀ , C. Tönnis ₅₇ , S. Toscano ₃ , D. Tosi ₂₈ , A. Trettin ₂ , M. Tselengidou ₉ , C.F. Tung ₃₀ , A. Turcati ₄₁ , R. Turcotte ₁₃ , C.F. Turley ₈ , B. Ty ₂₈ , E. Unger ₂₇ , M.A. Unland Elorrieta ₂₉ , M. Usner ₂ , J. Vandenbroucke ₂₈ , W. Van Driessche ₃₆ , D. van Eijk ₂₈ , N. van Eijndhoven ₃₄ , J. van Santen ₂ , S. Verpoest ₃₆ , M. Vraeghe ₃₆ , C. Walck ₅ , A. Wallace ₄₃ , M. Wallraff ₁₁ , N. Wandkowsky ₂₈ , T.B. Watson ₄₈ , C. Weaver ₄₂ , A. Weindl ₁₃ , M.J. Weiss ₈ , J. Weldert ₁₅ , C. Wendt ₂₈ , J. Werthebach ₂₈ , B.J. Whelan ₄₃ , N. Whitehorn ₅₈ , K. Wiebe ₁₅ , C.H. Wiebusch ₁₁ , L. Wille ₂₈ , D.R. Williams ₅₀ , L. Wills ₅₁ , M. Wolf ₄₁ , J. Wood ₂₈ , T.R. Wood ₄₂ , K. Woschnagg ₁₆ , G. Wrede ₉ , D.L. Xu ₂₈ , X.W. Xu ₃₉ , Y. Xu ₄₉ , J.P. Yanez ₄₂ , G. Yodh ₁₄ , S. Yoshida ₄₆ , T. Yuan ₂₈ , M. Zöcklein ₁₁

Affiliation

Dept. of Physics and Astronomy, University of Canterbury, Private Bag 4800, Christchurch, New Zealand
DESY, D-15738 Zeuthen, Germany [7pt]\mbox
Université Libre de Bruxelles, Science Faculty CP230, B-1050 Brussels, Belgium
Niels Bohr Institute, University of Copenhagen, DK-2100 Copenhagen, Denmark
Oskar Klein Centre and Dept. of Physics, Stockholm University, SE-10691 Stockholm, Sweden
Département de physique nucléaire et corpusculaire, Université de Genève, CH-1211 Genève, Switzerland
Department of Physics, Marquette University, Milwaukee, WI, 53201, U.S.A.
Dept. of Physics, Pennsylvania State University, University Park, PA 16802, U.S.A.
Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, D-91058 Erlangen, Germany
Dept. of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139, U.S.A.
III. Physikalisches Institut, RWTH Aachen University, D-52056 Aachen, Germany
Physics Department, South Dakota School of Mines and Technology, Rapid City, SD 57701, U.S.A.
Karlsruhe Institute of Technology, Institut für Kernphysik, D-76021 Karlsruhe, Germany
Dept. of Physics and Astronomy, University of California, Irvine, CA 92697, U.S.A.
Institute of Physics, University of Mainz, Staudinger Weg 7, D-55099 Mainz, Germany
Dept. of Physics, University of California, Berkeley, CA 94720, U.S.A.
Dept. of Astronomy, Ohio State University, Columbus, OH 43210, U.S.A.
Dept. of Physics and Center for Cosmology and Astro-Particle Physics, Ohio State University, Columbus, OH 43210, U.S.A.
Dept. of Physics, University of Wuppertal, D-42119 Wuppertal, Germany
Fakultät für Physik & Astronomie, Ruhr-Universität Bochum, D-44780 Bochum, Germany
Dept. of Physics and Astronomy, University of Rochester, Rochester, NY 14627, U.S.A.
Dept. of Physics, University of Maryland, College Park, MD 20742, U.S.A.
Also at Università di Padova, I-35131 Padova, Italy
Dept. of Physics and Astronomy, University of Kansas, Lawrence, KS 66045, U.S.A.
Also at National Research Nuclear University, Moscow Engineering Physics Institute (MEPhI), Moscow 115409, Russia
Lawrence Berkeley National Laboratory, Berkeley, CA 94720, U.S.A.
Dept. of Physics and Astronomy, Uppsala University, Box 516, S-75120 Uppsala, Sweden
Dept. of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin, Madison, WI 53706, U.S.A.
Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, D-48149 Münster, Germany
School of Physics and Center for Relativistic Astrophysics, Georgia Institute of Technology, Atlanta, GA 30332, U.S.A.
Dept. of Physics, Sungkyunkwan University, Suwon 16419, Korea
SNOLAB, 1039 Regional Road 24, Creighton Mine 9, Lively, ON, Canada P3Y 1N2
Bartol Research Institute and Dept. of Physics and Astronomy, University of Delaware, Newark, DE 19716, U.S.A.
Vrije Universiteit Brussel (VUB), Dienst ELEM, B-1050 Brussels, Belgium
Dept. of Astronomy and Astrophysics, Pennsylvania State University, University Park, PA 16802, U.S.A.
Dept. of Physics and Astronomy, University of Gent, B-9000 Gent, Belgium
Institut für Physik, Humboldt-Universität zu Berlin, D-12489 Berlin, Germany
Dept. of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, U.S.A.
Dept. of Physics, Southern University, Baton Rouge, LA 70813, U.S.A.
Dept. of Astronomy, University of Wisconsin, Madison, WI 53706, U.S.A.
Physik-department, Technische Universität München, D-85748 Garching, Germany
Dept. of Physics, University of Alberta, Edmonton, Alberta, Canada T6G 2E1
Department of Physics, University of Adelaide, Adelaide, 5005, Australia
Dept. of Physics, TU Dortmund University, D-44221 Dortmund, Germany
Earthquake Research Institute, University of Tokyo, Bunkyo, Tokyo 113-0032, Japan
Dept. of Physics and Institute for Global Prominent Research, Chiba University, Chiba 263-8522, Japan
CTSPS, Clark-Atlanta University, Atlanta, GA 30314, U.S.A.
Dept. of Physics, University of Texas at Arlington, 502 Yates St., Science Hall Rm 108, Box 19059, Arlington, TX 76019, U.S.A.
Dept. of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794-3800, U.S.A.
Dept. of Physics and Astronomy, University of Alabama, Tuscaloosa, AL 35487, U.S.A.
Dept. of Physics, Drexel University, 3141 Chestnut Street, Philadelphia, PA 19104, U.S.A.
Dept. of Physics, University of Wisconsin, River Falls, WI 54022, U.S.A.
Dept. of Physics, Yale University, New Haven, CT 06520, U.S.A.
Department of Physics, Mercer University, Macon, GA 31207-0001, U.S.A.
Dept. of Physics and Astronomy, University of Alaska Anchorage, 3211 Providence Dr., Anchorage, AK 99508, U.S.A.
Dept. of Physics, University of Oxford, Parks Road, Oxford OX1 3PU, U.K.
Institute of Basic Science, Sungkyunkwan University, Suwon 16419, Korea
Department of Physics and Astronomy, UCLA, Los Angeles, CA 90095, U.S.A.

The distribution of galaxies within the local universe is characterized by anisotropic features. Observatories searching for the production sites of astrophysical neutrinos can take advantage of these features to establish directional correlations between a neutrino dataset and overdensities in the galaxy distribution in the sky. The results of two correlation searches between a seven-year time-integrated neutrino dataset from the IceCube Neutrino Observatory, and the 2MASS Redshift Survey (2MRS) catalog are presented here. The first analysis searches for neutrinos produced via interactions between diffuse intergalactic Ultra-High Energy Cosmic Rays (UHECRs) and the matter contained within galaxies. The second analysis searches for low-luminosity sources within the local universe, which would produce subthreshold multiplets in the IceCube dataset that directionally correlate with galaxy distribution. No significant correlations were observed in either analyses. Constraints are presented on the flux of neutrinos originating within the local universe through diffuse intergalactic UHECR interactions, as well as on the density of standard candle sources of neutrinos at low luminosities.

中文翻译：

使用 2MASS 红移测量和 IceCube 对附近星系中微子发射的限制

本地宇宙中星系的分布具有各向异性特征。寻找天体物理中微子产生地点的天文台可以利用这些特征来建立中微子数据集与天空中星系分布密度之间的方向相关性。此处展示了来自 IceCube Neutrino Observatory 的 7 年时间积分中微子数据集与 2MASS Redshift Survey (2MRS) 目录之间的两次相关搜索结果。第一项分析搜索通过漫射星系际超高能宇宙射线 (UHECR) 与星系中所含物质之间的相互作用产生的中微子。第二个分析在本地宇宙中寻找低光度源，这将在 IceCube 数据集中产生与星系分布方向相关的亚阈值多重峰。在任一分析中均未观察到显着相关性。通过漫射星系间 UHECR 相互作用，以及低光度下中微子的标准烛光源密度，对源自本地宇宙的中微子通量提出了限制。

更新日期：2020-07-16

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