Properties of $Z_c^{\pm}(3900)$ produced in $p \bar p$ collision
D0 Collaboration

TL;DR
This paper investigates the production and properties of the exotic $Z_c^{\u2212}(3900)$ state in proton-antiproton collisions, measuring its mass and width, and setting limits on its prompt production relative to $b$-hadron decays.
Contribution
It provides the first measurement of the $Z_c^{\u2212}(3900)$ mass and width in $p ar p$ collisions and searches for its prompt production, establishing upper limits.
Findings
Measured $Z_c^{\u2212}(3900)$ mass as 3902.6 MeV
Determined the width to be approximately 32 MeV
Set an upper limit of 0.66 on prompt production ratio
Abstract
We study the production of the exotic charged charmonium-like state in collisions through the sequential process , . Using the subsample of candidates originating from semi-inclusive weak decays of -flavored hadrons, we measure the invariant mass and natural width to be MeV and MeV, respectively. We search for prompt production of the through the same sequential process. No significant signal is observed, and we set an upper limit of 0.66 at the 95\% credibility level on the ratio of prompt production to the production via -hadron decays. The study is based on…
| Displaced vertex | Primary vertex | |||||
|---|---|---|---|---|---|---|
| GeV | Event yield | () | Event yield | () | ||
| 4.1–4.2 | 18.7/14 | 1.3 | 52.7/15 | 0.9 | ||
| 4.2–4.3 | 28.1/16 | 5.2 | 21.9/14 | 0.5 | ||
| 4.3–4.4 | 17.4/15 | 2.3 | 16.7/19 | 1.1 | ||
| 4.4–4.5 | 26.6/15 | 0.5 | 30.9/18 | 1.5 | ||
| 4.5–4.6 | 23.7/25 | 1.7 | 42.3/23 | 1.4 | ||
| 4.6–4.7 | 57.4/25 | 1.4 | 46.3/23 | 2.2 |
| Source | Mass, MeV | Width, MeV | |
|---|---|---|---|
| Mass calibration | |||
| Mass resolution | 0.1 | ||
| Background shape | |||
| Total (sum in quadrature) |
| Source | Displaced vertex | Primary vertex | |
|---|---|---|---|
| Mass resolution | 18 | 18 | |
| Trigger bias | 19 | – | |
| Acceptance | 7 | – | |
| Signal mass | 11 | ||
| Signal width | |||
| Background shape | 2 | ||
| Total (sum in quadrature) |
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FERMILAB-PUB-19-253-E Published in Phys. Rev. D as DOI: 10.1103/PhysRevD.100.012005
The D0 Collaboration111with visitors from aAugustana College, Sioux Falls, SD 57197, USA, bThe University of Liverpool, Liverpool L69 3BX, UK, cDeutshes Elektronen-Synchrotron (DESY), Notkestrasse 85, Germany, dCONACyT, M-03940 Mexico City, Mexico, eSLAC, Menlo Park, CA 94025, USA, fUniversity College London, London WC1E 6BT, UK, gCentro de Investigacion en Computacion - IPN, CP 07738 Mexico City, Mexico, hUniversidade Estadual Paulista, São Paulo, SP 01140, Brazil, iKarlsruher Institut für Technologie (KIT) - Steinbuch Centre for Computing (SCC), D-76128 Karlsruhe, Germany, jOffice of Science, U.S. Department of Energy, Washington, D.C. 20585, USA, lKiev Institute for Nuclear Research (KINR), Kyiv 03680, Ukraine, mUniversity of Maryland, College Park, MD 20742, USA, nEuropean Orgnaization for Nuclear Research (CERN), CH-1211 Geneva, Switzerland, oPurdue University, West Lafayette, IN 47907, USA, pInstitute of Physics, Belgrade, Belgrade, Serbia, and qP.N. Lebedev Physical Institute of the Russian Academy of Sciences, 119991, Moscow, Russia. *‡*Deceased.
Properties of produced in collisions
V.M. Abazov
Joint Institute for Nuclear Research, Dubna 141980, Russia
B. Abbott
University of Oklahoma, Norman, Oklahoma 73019, USA
B.S. Acharya
Tata Institute of Fundamental Research, Mumbai-400 005, India
M. Adams
University of Illinois at Chicago, Chicago, Illinois 60607, USA
T. Adams
Florida State University, Tallahassee, Florida 32306, USA
J.P. Agnew
The University of Manchester, Manchester M13 9PL, United Kingdom
G.D. Alexeev
Joint Institute for Nuclear Research, Dubna 141980, Russia
G. Alkhazov
Petersburg Nuclear Physics Institute, St. Petersburg 188300, Russia
A. Altona
University of Michigan, Ann Arbor, Michigan 48109, USA
A. Askew
Florida State University, Tallahassee, Florida 32306, USA
S. Atkins
Louisiana Tech University, Ruston, Louisiana 71272, USA
K. Augsten
Czech Technical University in Prague, 116 36 Prague 6, Czech Republic
V. Aushev
Taras Shevchenko National University of Kyiv, Kiev, 01601, Ukraine
Y. Aushev
Taras Shevchenko National University of Kyiv, Kiev, 01601, Ukraine
C. Avila
Universidad de los Andes, Bogotá, 111711, Colombia
F. Badaud
LPC, Université Blaise Pascal, CNRS/IN2P3, Clermont, F-63178 Aubière Cedex, France
L. Bagby
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
B. Baldin
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
D.V. Bandurin
University of Virginia, Charlottesville, Virginia 22904, USA
S. Banerjee
Tata Institute of Fundamental Research, Mumbai-400 005, India
E. Barberis
Northeastern University, Boston, Massachusetts 02115, USA
P. Baringer
University of Kansas, Lawrence, Kansas 66045, USA
J.F. Bartlett
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
U. Bassler
CEA Saclay, Irfu, SPP, F-91191 Gif-Sur-Yvette Cedex, France
V. Bazterra
University of Illinois at Chicago, Chicago, Illinois 60607, USA
A. Bean
University of Kansas, Lawrence, Kansas 66045, USA
M. Begalli
Universidade do Estado do Rio de Janeiro, Rio de Janeiro, RJ 20550, Brazil
L. Bellantoni
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
S.B. Beri
Panjab University, Chandigarh 160014, India
G. Bernardi
LPNHE, Universités Paris VI and VII, CNRS/IN2P3, F-75005 Paris, France
R. Bernhard
Physikalisches Institut, Universität Freiburg, 79085 Freiburg, Germany
I. Bertram
Lancaster University, Lancaster LA1 4YB, United Kingdom
M. Besançon
CEA Saclay, Irfu, SPP, F-91191 Gif-Sur-Yvette Cedex, France
R. Beuselinck
Imperial College London, London SW7 2AZ, United Kingdom
P.C. Bhat
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
S. Bhatia
University of Mississippi, University, Mississippi 38677, USA
V. Bhatnagar
Panjab University, Chandigarh 160014, India
G. Blazey
Northern Illinois University, DeKalb, Illinois 60115, USA
S. Blessing
Florida State University, Tallahassee, Florida 32306, USA
K. Bloom
University of Nebraska, Lincoln, Nebraska 68588, USA
A. Boehnlein
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
D. Boline
State University of New York, Stony Brook, New York 11794, USA
E.E. Boos
Moscow State University, Moscow 119991, Russia
G. Borissov
Lancaster University, Lancaster LA1 4YB, United Kingdom
M. Borysoval
Taras Shevchenko National University of Kyiv, Kiev, 01601, Ukraine
A. Brandt
University of Texas, Arlington, Texas 76019, USA
O. Brandt
II. Physikalisches Institut, Georg-August-Universität Göttingen, 37073 Göttingen, Germany
M. Brochmann
University of Washington, Seattle, Washington 98195, USA
R. Brock
Michigan State University, East Lansing, Michigan 48824, USA
A. Bross
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
D. Brown
LPNHE, Universités Paris VI and VII, CNRS/IN2P3, F-75005 Paris, France
X.B. Bu
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
M. Buehler
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
V. Buescher
Institut für Physik, Universität Mainz, 55099 Mainz, Germany
V. Bunichev
Moscow State University, Moscow 119991, Russia
S. Burdinb
Lancaster University, Lancaster LA1 4YB, United Kingdom
C.P. Buszello
Uppsala University, 751 05 Uppsala, Sweden
E. Camacho-Pérez
CINVESTAV, Mexico City 07360, Mexico
B.C.K. Casey
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
H. Castilla-Valdez
CINVESTAV, Mexico City 07360, Mexico
S. Caughron
Michigan State University, East Lansing, Michigan 48824, USA
S. Chakrabarti
State University of New York, Stony Brook, New York 11794, USA
K.M. Chan
University of Notre Dame, Notre Dame, Indiana 46556, USA
A. Chandra
Rice University, Houston, Texas 77005, USA
E. Chapon
CEA Saclay, Irfu, SPP, F-91191 Gif-Sur-Yvette Cedex, France
G. Chen
University of Kansas, Lawrence, Kansas 66045, USA
S.W. Cho
Korea Detector Laboratory, Korea University, Seoul, 02841, Korea
S. Choi
Korea Detector Laboratory, Korea University, Seoul, 02841, Korea
B. Choudhary
Delhi University, Delhi-110 007, India
S. Cihangir*‡*
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
D. Claes
University of Nebraska, Lincoln, Nebraska 68588, USA
J. Clutter
University of Kansas, Lawrence, Kansas 66045, USA
M. Cookej
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
W.E. Cooper
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
M. Corcoran*‡*
Rice University, Houston, Texas 77005, USA
F. Couderc
CEA Saclay, Irfu, SPP, F-91191 Gif-Sur-Yvette Cedex, France
M.-C. Cousinou
CPPM, Aix-Marseille Université, CNRS/IN2P3, F-13288 Marseille Cedex 09, France
J. Cuth
Institut für Physik, Universität Mainz, 55099 Mainz, Germany
D. Cutts
Brown University, Providence, Rhode Island 02912, USA
A. Das
Southern Methodist University, Dallas, Texas 75275, USA
G. Davies
Imperial College London, London SW7 2AZ, United Kingdom
S.J. de Jong
Nikhef, Science Park, 1098 XG Amsterdam, the Netherlands
Radboud University Nijmegen, 6525 AJ Nijmegen, the Netherlands
E. De La Cruz-Burelo
CINVESTAV, Mexico City 07360, Mexico
F. Déliot
CEA Saclay, Irfu, SPP, F-91191 Gif-Sur-Yvette Cedex, France
R. Demina
University of Rochester, Rochester, New York 14627, USA
D. Denisov
Brookhaven National Laboratory, Upton, New York 11973, USA
S.P. Denisov
Institute for High Energy Physics, Protvino, Moscow region 142281, Russia
S. Desai
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
C. Deterrec
The University of Manchester, Manchester M13 9PL, United Kingdom
K. DeVaughan
University of Nebraska, Lincoln, Nebraska 68588, USA
H.T. Diehl
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
M. Diesburg
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
P.F. Ding
The University of Manchester, Manchester M13 9PL, United Kingdom
A. Dominguez
University of Nebraska, Lincoln, Nebraska 68588, USA
A. Drutskoyq
Institute for Theoretical and Experimental Physics, Moscow 117259, Russia
A. Dubey
Delhi University, Delhi-110 007, India
L.V. Dudko
Moscow State University, Moscow 119991, Russia
A. Duperrin
CPPM, Aix-Marseille Université, CNRS/IN2P3, F-13288 Marseille Cedex 09, France
S. Dutt
Panjab University, Chandigarh 160014, India
M. Eads
Northern Illinois University, DeKalb, Illinois 60115, USA
D. Edmunds
Michigan State University, East Lansing, Michigan 48824, USA
J. Ellison
University of California Riverside, Riverside, California 92521, USA
V.D. Elvira
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
Y. Enari
LPNHE, Universités Paris VI and VII, CNRS/IN2P3, F-75005 Paris, France
H. Evans
Indiana University, Bloomington, Indiana 47405, USA
A. Evdokimov
University of Illinois at Chicago, Chicago, Illinois 60607, USA
V.N. Evdokimov
Institute for High Energy Physics, Protvino, Moscow region 142281, Russia
A. Fauré
CEA Saclay, Irfu, SPP, F-91191 Gif-Sur-Yvette Cedex, France
L. Feng
Northern Illinois University, DeKalb, Illinois 60115, USA
T. Ferbel
University of Rochester, Rochester, New York 14627, USA
F. Fiedler
Institut für Physik, Universität Mainz, 55099 Mainz, Germany
F. Filthaut
Nikhef, Science Park, 1098 XG Amsterdam, the Netherlands
Radboud University Nijmegen, 6525 AJ Nijmegen, the Netherlands
W. Fisher
Michigan State University, East Lansing, Michigan 48824, USA
H.E. Fisk
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
M. Fortner
Northern Illinois University, DeKalb, Illinois 60115, USA
H. Fox
Lancaster University, Lancaster LA1 4YB, United Kingdom
J. Franc
Czech Technical University in Prague, 116 36 Prague 6, Czech Republic
S. Fuess
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
P.H. Garbincius
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
A. Garcia-Bellido
University of Rochester, Rochester, New York 14627, USA
J.A. García-González
CINVESTAV, Mexico City 07360, Mexico
V. Gavrilov
Institute for Theoretical and Experimental Physics, Moscow 117259, Russia
W. Geng
CPPM, Aix-Marseille Université, CNRS/IN2P3, F-13288 Marseille Cedex 09, France
Michigan State University, East Lansing, Michigan 48824, USA
C.E. Gerber
University of Illinois at Chicago, Chicago, Illinois 60607, USA
Y. Gershtein
Rutgers University, Piscataway, New Jersey 08855, USA
G. Ginther
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
O. Gogota
Taras Shevchenko National University of Kyiv, Kiev, 01601, Ukraine
G. Golovanov
Joint Institute for Nuclear Research, Dubna 141980, Russia
P.D. Grannis
State University of New York, Stony Brook, New York 11794, USA
S. Greder
IPHC, Université de Strasbourg, CNRS/IN2P3, F-67037 Strasbourg, France
H. Greenlee
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
G. Grenier
IPNL, Université Lyon 1, CNRS/IN2P3, F-69622 Villeurbanne Cedex, France and Université de Lyon, F-69361 Lyon CEDEX 07, France
Ph. Gris
LPC, Université Blaise Pascal, CNRS/IN2P3, Clermont, F-63178 Aubière Cedex, France
J.-F. Grivaz
LAL, Univ. Paris-Sud, CNRS/IN2P3, Université Paris-Saclay, F-91898 Orsay Cedex, France
A. Grohsjeanc
CEA Saclay, Irfu, SPP, F-91191 Gif-Sur-Yvette Cedex, France
S. Grünendahl
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
M.W. Grünewald
University College Dublin, Dublin 4, Ireland
T. Guillemin
LAL, Univ. Paris-Sud, CNRS/IN2P3, Université Paris-Saclay, F-91898 Orsay Cedex, France
G. Gutierrez
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
P. Gutierrez
University of Oklahoma, Norman, Oklahoma 73019, USA
J. Haley
Oklahoma State University, Stillwater, Oklahoma 74078, USA
L. Han
University of Science and Technology of China, Hefei 230026, People’s Republic of China
K. Harder
The University of Manchester, Manchester M13 9PL, United Kingdom
A. Harel
University of Rochester, Rochester, New York 14627, USA
J.M. Hauptman
Iowa State University, Ames, Iowa 50011, USA
J. Hays
Imperial College London, London SW7 2AZ, United Kingdom
T. Head
The University of Manchester, Manchester M13 9PL, United Kingdom
T. Hebbeker
III. Physikalisches Institut A, RWTH Aachen University, 52056 Aachen, Germany
D. Hedin
Northern Illinois University, DeKalb, Illinois 60115, USA
H. Hegab
Oklahoma State University, Stillwater, Oklahoma 74078, USA
A.P. Heinson
University of California Riverside, Riverside, California 92521, USA
U. Heintz
Brown University, Providence, Rhode Island 02912, USA
C. Hensel
LAFEX, Centro Brasileiro de Pesquisas Físicas, Rio de Janeiro, RJ 22290, Brazil
I. Heredia-De La Cruzd
CINVESTAV, Mexico City 07360, Mexico
K. Herner
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
G. Heskethf
The University of Manchester, Manchester M13 9PL, United Kingdom
M.D. Hildreth
University of Notre Dame, Notre Dame, Indiana 46556, USA
R. Hirosky
University of Virginia, Charlottesville, Virginia 22904, USA
T. Hoang
Florida State University, Tallahassee, Florida 32306, USA
J.D. Hobbs
State University of New York, Stony Brook, New York 11794, USA
B. Hoeneisen
Universidad San Francisco de Quito, Quito 170157, Ecuador
J. Hogan
Rice University, Houston, Texas 77005, USA
M. Hohlfeld
Institut für Physik, Universität Mainz, 55099 Mainz, Germany
J.L. Holzbauer
University of Mississippi, University, Mississippi 38677, USA
I. Howley
University of Texas, Arlington, Texas 76019, USA
Z. Hubacek
Czech Technical University in Prague, 116 36 Prague 6, Czech Republic
CEA Saclay, Irfu, SPP, F-91191 Gif-Sur-Yvette Cedex, France
V. Hynek
Czech Technical University in Prague, 116 36 Prague 6, Czech Republic
I. Iashvili
State University of New York, Buffalo, New York 14260, USA
Y. Ilchenko
Southern Methodist University, Dallas, Texas 75275, USA
R. Illingworth
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
A.S. Ito
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
S. Jabeenm
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
M. Jaffré
LAL, Univ. Paris-Sud, CNRS/IN2P3, Université Paris-Saclay, F-91898 Orsay Cedex, France
A. Jayasinghe
University of Oklahoma, Norman, Oklahoma 73019, USA
M.S. Jeong
Korea Detector Laboratory, Korea University, Seoul, 02841, Korea
R. Jesik
Imperial College London, London SW7 2AZ, United Kingdom
P. Jiang*‡*
University of Science and Technology of China, Hefei 230026, People’s Republic of China
K. Johns
University of Arizona, Tucson, Arizona 85721, USA
E. Johnson
Michigan State University, East Lansing, Michigan 48824, USA
M. Johnson
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
A. Jonckheere
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
P. Jonsson
Imperial College London, London SW7 2AZ, United Kingdom
J. Joshi
University of California Riverside, Riverside, California 92521, USA
A.W. Jungo
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
A. Juste
Institució Catalana de Recerca i Estudis Avançats (ICREA) and Institut de Física d’Altes Energies (IFAE), 08193 Bellaterra (Barcelona), Spain
E. Kajfasz
CPPM, Aix-Marseille Université, CNRS/IN2P3, F-13288 Marseille Cedex 09, France
D. Karmanov
Moscow State University, Moscow 119991, Russia
I. Katsanos
University of Nebraska, Lincoln, Nebraska 68588, USA
M. Kaur
Panjab University, Chandigarh 160014, India
R. Kehoe
Southern Methodist University, Dallas, Texas 75275, USA
S. Kermiche
CPPM, Aix-Marseille Université, CNRS/IN2P3, F-13288 Marseille Cedex 09, France
N. Khalatyan
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
A. Khanov
Oklahoma State University, Stillwater, Oklahoma 74078, USA
A. Kharchilava
State University of New York, Buffalo, New York 14260, USA
Y.N. Kharzheev
Joint Institute for Nuclear Research, Dubna 141980, Russia
I. Kiselevich
Institute for Theoretical and Experimental Physics, Moscow 117259, Russia
J.M. Kohli
Panjab University, Chandigarh 160014, India
A.V. Kozelov
Institute for High Energy Physics, Protvino, Moscow region 142281, Russia
J. Kraus
University of Mississippi, University, Mississippi 38677, USA
A. Kumar
State University of New York, Buffalo, New York 14260, USA
A. Kupco
Institute of Physics, Academy of Sciences of the Czech Republic, 182 21 Prague, Czech Republic
T. Kurča
IPNL, Université Lyon 1, CNRS/IN2P3, F-69622 Villeurbanne Cedex, France and Université de Lyon, F-69361 Lyon CEDEX 07, France
V.A. Kuzmin
Moscow State University, Moscow 119991, Russia
S. Lammers
Indiana University, Bloomington, Indiana 47405, USA
P. Lebrun
IPNL, Université Lyon 1, CNRS/IN2P3, F-69622 Villeurbanne Cedex, France and Université de Lyon, F-69361 Lyon CEDEX 07, France
H.S. Lee
Korea Detector Laboratory, Korea University, Seoul, 02841, Korea
S.W. Lee
Iowa State University, Ames, Iowa 50011, USA
W.M. Lee*‡*
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
X. Lei
University of Arizona, Tucson, Arizona 85721, USA
J. Lellouch
LPNHE, Universités Paris VI and VII, CNRS/IN2P3, F-75005 Paris, France
D. Li
LPNHE, Universités Paris VI and VII, CNRS/IN2P3, F-75005 Paris, France
H. Li
University of Virginia, Charlottesville, Virginia 22904, USA
L. Li
University of California Riverside, Riverside, California 92521, USA
Q.Z. Li
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
J.K. Lim
Korea Detector Laboratory, Korea University, Seoul, 02841, Korea
D. Lincoln
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
J. Linnemann
Michigan State University, East Lansing, Michigan 48824, USA
V.V. Lipaev*‡*
Institute for High Energy Physics, Protvino, Moscow region 142281, Russia
R. Lipton
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
H. Liu
Southern Methodist University, Dallas, Texas 75275, USA
Y. Liu
University of Science and Technology of China, Hefei 230026, People’s Republic of China
A. Lobodenko
Petersburg Nuclear Physics Institute, St. Petersburg 188300, Russia
M. Lokajicek
Institute of Physics, Academy of Sciences of the Czech Republic, 182 21 Prague, Czech Republic
R. Lopes de Sa
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
R. Luna-Garciag
CINVESTAV, Mexico City 07360, Mexico
A.L. Lyon
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
A.K.A. Maciel
LAFEX, Centro Brasileiro de Pesquisas Físicas, Rio de Janeiro, RJ 22290, Brazil
R. Madar
Physikalisches Institut, Universität Freiburg, 79085 Freiburg, Germany
R. Magaña-Villalba
CINVESTAV, Mexico City 07360, Mexico
S. Malik
University of Nebraska, Lincoln, Nebraska 68588, USA
V.L. Malyshev
Joint Institute for Nuclear Research, Dubna 141980, Russia
J. Mansour
II. Physikalisches Institut, Georg-August-Universität Göttingen, 37073 Göttingen, Germany
J. Martínez-Ortega
CINVESTAV, Mexico City 07360, Mexico
R. McCarthy
State University of New York, Stony Brook, New York 11794, USA
C.L. McGivern
The University of Manchester, Manchester M13 9PL, United Kingdom
M.M. Meijer
Nikhef, Science Park, 1098 XG Amsterdam, the Netherlands
Radboud University Nijmegen, 6525 AJ Nijmegen, the Netherlands
A. Melnitchouk
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
D. Menezes
Northern Illinois University, DeKalb, Illinois 60115, USA
P.G. Mercadante
Universidade Federal do ABC, Santo André, SP 09210, Brazil
M. Merkin
Moscow State University, Moscow 119991, Russia
A. Meyer
III. Physikalisches Institut A, RWTH Aachen University, 52056 Aachen, Germany
J. Meyeri
II. Physikalisches Institut, Georg-August-Universität Göttingen, 37073 Göttingen, Germany
F. Miconi
IPHC, Université de Strasbourg, CNRS/IN2P3, F-67037 Strasbourg, France
N.K. Mondal
Tata Institute of Fundamental Research, Mumbai-400 005, India
M. Mulhearn
University of Virginia, Charlottesville, Virginia 22904, USA
E. Nagy
CPPM, Aix-Marseille Université, CNRS/IN2P3, F-13288 Marseille Cedex 09, France
M. Narain
Brown University, Providence, Rhode Island 02912, USA
R. Nayyar
University of Arizona, Tucson, Arizona 85721, USA
H.A. Neal*‡*
University of Michigan, Ann Arbor, Michigan 48109, USA
J.P. Negret
Universidad de los Andes, Bogotá, 111711, Colombia
P. Neustroev
Petersburg Nuclear Physics Institute, St. Petersburg 188300, Russia
H.T. Nguyen
University of Virginia, Charlottesville, Virginia 22904, USA
T. Nunnemann
Ludwig-Maximilians-Universität München, 80539 München, Germany
J. Orduna
Brown University, Providence, Rhode Island 02912, USA
N. Osman
CPPM, Aix-Marseille Université, CNRS/IN2P3, F-13288 Marseille Cedex 09, France
A. Pal
University of Texas, Arlington, Texas 76019, USA
N. Parashar
Purdue University Calumet, Hammond, Indiana 46323, USA
V. Parihar
Brown University, Providence, Rhode Island 02912, USA
S.K. Park
Korea Detector Laboratory, Korea University, Seoul, 02841, Korea
R. Partridgee
Brown University, Providence, Rhode Island 02912, USA
N. Parua
Indiana University, Bloomington, Indiana 47405, USA
A. Patwaj
Brookhaven National Laboratory, Upton, New York 11973, USA
B. Penning
Imperial College London, London SW7 2AZ, United Kingdom
M. Perfilov
Moscow State University, Moscow 119991, Russia
Y. Peters
The University of Manchester, Manchester M13 9PL, United Kingdom
K. Petridis
The University of Manchester, Manchester M13 9PL, United Kingdom
G. Petrillo
University of Rochester, Rochester, New York 14627, USA
P. Pétroff
LAL, Univ. Paris-Sud, CNRS/IN2P3, Université Paris-Saclay, F-91898 Orsay Cedex, France
M.-A. Pleier
Brookhaven National Laboratory, Upton, New York 11973, USA
V.M. Podstavkov
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
A.V. Popov
Institute for High Energy Physics, Protvino, Moscow region 142281, Russia
M. Prewitt
Rice University, Houston, Texas 77005, USA
D. Price
The University of Manchester, Manchester M13 9PL, United Kingdom
N. Prokopenko
Institute for High Energy Physics, Protvino, Moscow region 142281, Russia
J. Qian
University of Michigan, Ann Arbor, Michigan 48109, USA
A. Quadt
II. Physikalisches Institut, Georg-August-Universität Göttingen, 37073 Göttingen, Germany
B. Quinn
University of Mississippi, University, Mississippi 38677, USA
P.N. Ratoff
Lancaster University, Lancaster LA1 4YB, United Kingdom
I. Razumov
Institute for High Energy Physics, Protvino, Moscow region 142281, Russia
I. Ripp-Baudot
IPHC, Université de Strasbourg, CNRS/IN2P3, F-67037 Strasbourg, France
F. Rizatdinova
Oklahoma State University, Stillwater, Oklahoma 74078, USA
M. Rominsky
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
A. Ross
Lancaster University, Lancaster LA1 4YB, United Kingdom
C. Royon
Institute of Physics, Academy of Sciences of the Czech Republic, 182 21 Prague, Czech Republic
P. Rubinov
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
R. Ruchti
University of Notre Dame, Notre Dame, Indiana 46556, USA
G. Sajot
LPSC, Université Joseph Fourier Grenoble 1, CNRS/IN2P3, Institut National Polytechnique de Grenoble, F-38026 Grenoble Cedex, France
A. Sánchez-Hernández
CINVESTAV, Mexico City 07360, Mexico
M.P. Sanders
Ludwig-Maximilians-Universität München, 80539 München, Germany
A.S. Santosh
LAFEX, Centro Brasileiro de Pesquisas Físicas, Rio de Janeiro, RJ 22290, Brazil
G. Savage
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
M. Savitskyi
Taras Shevchenko National University of Kyiv, Kiev, 01601, Ukraine
L. Sawyer
Louisiana Tech University, Ruston, Louisiana 71272, USA
T. Scanlon
Imperial College London, London SW7 2AZ, United Kingdom
R.D. Schamberger
State University of New York, Stony Brook, New York 11794, USA
Y. Scheglov*‡*
Petersburg Nuclear Physics Institute, St. Petersburg 188300, Russia
H. Schellman
Oregon State University, Corvallis, Oregon 97331, USA
Northwestern University, Evanston, Illinois 60208, USA
M. Schott
Institut für Physik, Universität Mainz, 55099 Mainz, Germany
C. Schwanenberger
The University of Manchester, Manchester M13 9PL, United Kingdom
R. Schwienhorst
Michigan State University, East Lansing, Michigan 48824, USA
J. Sekaric
University of Kansas, Lawrence, Kansas 66045, USA
H. Severini
University of Oklahoma, Norman, Oklahoma 73019, USA
E. Shabalina
II. Physikalisches Institut, Georg-August-Universität Göttingen, 37073 Göttingen, Germany
V. Shary
CEA Saclay, Irfu, SPP, F-91191 Gif-Sur-Yvette Cedex, France
S. Shaw
The University of Manchester, Manchester M13 9PL, United Kingdom
A.A. Shchukin
Institute for High Energy Physics, Protvino, Moscow region 142281, Russia
O. Shkola
Taras Shevchenko National University of Kyiv, Kiev, 01601, Ukraine
V. Simak
Czech Technical University in Prague, 116 36 Prague 6, Czech Republic
P. Skubic
University of Oklahoma, Norman, Oklahoma 73019, USA
P. Slattery
University of Rochester, Rochester, New York 14627, USA
G.R. Snow*‡*
University of Nebraska, Lincoln, Nebraska 68588, USA
J. Snow
Langston University, Langston, Oklahoma 73050, USA
S. Snyder
Brookhaven National Laboratory, Upton, New York 11973, USA
S. Söldner-Rembold
The University of Manchester, Manchester M13 9PL, United Kingdom
L. Sonnenschein
III. Physikalisches Institut A, RWTH Aachen University, 52056 Aachen, Germany
K. Soustruznik
Charles University, Faculty of Mathematics and Physics, Center for Particle Physics, 116 36 Prague 1, Czech Republic
J. Stark
LPSC, Université Joseph Fourier Grenoble 1, CNRS/IN2P3, Institut National Polytechnique de Grenoble, F-38026 Grenoble Cedex, France
N. Stefaniuk
Taras Shevchenko National University of Kyiv, Kiev, 01601, Ukraine
D.A. Stoyanova
Institute for High Energy Physics, Protvino, Moscow region 142281, Russia
M. Strauss
University of Oklahoma, Norman, Oklahoma 73019, USA
L. Suter
The University of Manchester, Manchester M13 9PL, United Kingdom
P. Svoisky
University of Virginia, Charlottesville, Virginia 22904, USA
M. Titov
CEA Saclay, Irfu, SPP, F-91191 Gif-Sur-Yvette Cedex, France
V.V. Tokmenin
Joint Institute for Nuclear Research, Dubna 141980, Russia
Y.-T. Tsai
University of Rochester, Rochester, New York 14627, USA
D. Tsybychev
State University of New York, Stony Brook, New York 11794, USA
B. Tuchming
CEA Saclay, Irfu, SPP, F-91191 Gif-Sur-Yvette Cedex, France
C. Tully
Princeton University, Princeton, New Jersey 08544, USA
L. Uvarov
Petersburg Nuclear Physics Institute, St. Petersburg 188300, Russia
S. Uvarov
Petersburg Nuclear Physics Institute, St. Petersburg 188300, Russia
S. Uzunyan
Northern Illinois University, DeKalb, Illinois 60115, USA
R. Van Kooten
Indiana University, Bloomington, Indiana 47405, USA
W.M. van Leeuwen
Nikhef, Science Park, 1098 XG Amsterdam, the Netherlands
N. Varelas
University of Illinois at Chicago, Chicago, Illinois 60607, USA
E.W. Varnes
University of Arizona, Tucson, Arizona 85721, USA
I.A. Vasilyev
Institute for High Energy Physics, Protvino, Moscow region 142281, Russia
A.Y. Verkheev
Joint Institute for Nuclear Research, Dubna 141980, Russia
L.S. Vertogradov
Joint Institute for Nuclear Research, Dubna 141980, Russia
M. Verzocchi
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
M. Vesterinen
The University of Manchester, Manchester M13 9PL, United Kingdom
D. Vilanova
CEA Saclay, Irfu, SPP, F-91191 Gif-Sur-Yvette Cedex, France
P. Vokac
Czech Technical University in Prague, 116 36 Prague 6, Czech Republic
H.D. Wahl
Florida State University, Tallahassee, Florida 32306, USA
M.H.L.S. Wang
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
J. Warchol*‡*
University of Notre Dame, Notre Dame, Indiana 46556, USA
G. Watts
University of Washington, Seattle, Washington 98195, USA
M. Wayne
University of Notre Dame, Notre Dame, Indiana 46556, USA
J. Weichert
Institut für Physik, Universität Mainz, 55099 Mainz, Germany
L. Welty-Rieger
Northwestern University, Evanston, Illinois 60208, USA
M.R.J. Williamsn
Indiana University, Bloomington, Indiana 47405, USA
G.W. Wilson
University of Kansas, Lawrence, Kansas 66045, USA
M. Wobisch
Louisiana Tech University, Ruston, Louisiana 71272, USA
D.R. Wood
Northeastern University, Boston, Massachusetts 02115, USA
T.R. Wyatt
The University of Manchester, Manchester M13 9PL, United Kingdom
Y. Xie
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
R. Yamada
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
S. Yang
University of Science and Technology of China, Hefei 230026, People’s Republic of China
T. Yasuda
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
Y.A. Yatsunenko
Joint Institute for Nuclear Research, Dubna 141980, Russia
W. Ye
State University of New York, Stony Brook, New York 11794, USA
Z. Ye
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
H. Yin
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
K. Yip
Brookhaven National Laboratory, Upton, New York 11973, USA
S.W. Youn
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
J.M. Yu
University of Michigan, Ann Arbor, Michigan 48109, USA
J. Zennamo
State University of New York, Buffalo, New York 14260, USA
T.G. Zhao
The University of Manchester, Manchester M13 9PL, United Kingdom
B. Zhou
University of Michigan, Ann Arbor, Michigan 48109, USA
J. Zhu
University of Michigan, Ann Arbor, Michigan 48109, USA
M. Zielinski
University of Rochester, Rochester, New York 14627, USA
D. Zieminska
Indiana University, Bloomington, Indiana 47405, USA
L. Zivkovicp
LPNHE, Universités Paris VI and VII, CNRS/IN2P3, F-75005 Paris, France
(May 31, 2019)
Abstract
We study the production of the exotic charged charmonium-like state in collisions through the sequential process , . Using the subsample of candidates originating from semi-inclusive weak decays of -flavored hadrons, we measure the invariant mass and natural width to be MeV and MeV, respectively. We search for prompt production of the through the same sequential process. No significant signal is observed, and we set an upper limit of 0.70 at the 95% credibility level on the ratio of prompt production to the production via -hadron decays. The study is based on of collision data collected by the D0 experiment at the Fermilab Tevatron collider.
I Introduction
In high-energy hadron collisions, charmonium is known to be produced both promptly in QCD processes and non-promptly in -hadron decays, with well measured rates. For both and mesons the non-prompt fraction increases with transverse momentum but prompt production dominates in most of the studied range fb .
Much less information exists about the hadronic production of exotic multiquark states containing a charm quark and antiquark. The – the most extensively studied exotic meson – is produced copiously in prompt interactions at TeV d03872 , and in collisions at TeV 7tev3872 and TeV 8tev3872 . The fraction of the inclusive production rate of the mesons originating from decays of -flavored hadrons () is found to be approximately 0.3 7tev3872 ; 8tev3872 , independent of . Evidence for prompt production of the , another exotic candidate, was also reported by D0 d04140 . The large prompt production rate of the has often been used as an argument against its identification as a weakly bound charm-meson molecule; see Ref. bra3872 for the latest discussion.
In Ref. zc1 , the D0 Collaboration presented the first evidence for production of the manifestly exotic charmonium-like state in semi-inclusive weak decays of -flavored hadrons in events containing a non-prompt and a pair of oppositely charged particles, assumed to be pions. That analysis considered the mass range GeV that includes the state: , , . This article presents an extension of that study to a search for prompt production of the through the sequential process , . The event sample used in this analysis is approximately 50% larger than in Ref. zc1 due to the use of an extended track finding algorithm optimized for reconstructing low- tracks.
II The D0 detector, event reconstruction, and selection
The D0 detector has a central tracking system consisting of a silicon microstrip tracker and a central fiber tracker, both located within a 1.9 T superconducting solenoidal magnet d0det ; layer0 . A muon system, covering eta , consists of a layer of tracking detectors and scintillation trigger counters in front of a central and two forward 1.8 T iron toroidal magnets, followed by two similar layers after the toroids run2muon . Events used in this analysis are collected with both single-muon and dimuon triggers. Single-muon triggers require a coincidence of signals in trigger elements inside and outside the toroidal magnets. All dimuon triggers require at least one muon to have track segments after the toroid; muons in the forward region are always required to penetrate the toroid.
The minimum muon transverse momentum is 1.5 GeV. No minimum requirement is applied to the muon pair, but the effective threshold is approximately 4 GeV due to the requirement for muons to penetrate the toroids, and the average value for accepted events is 10 GeV.
In collisions the is produced promptly, either directly or in strong decays of higher-mass charmonium states, or non-promptly in -hadron decays. Prompt mesons have a decay vertex consistent with the interaction point while those from the decays are displaced on average by (1 mm) as a result of the long -hadron lifetime.
We reconstruct decay candidates accompanied by a pair of charged particles, assumed to be pions, with opposite charges and with GeV. We perform a kinematic fit under the hypothesis that the muons come from the and that the and the two particles originate from the same space point. In the fit, the dimuon invariant mass is constrained to the world-average value of the meson mass pdg . The track parameters (, position and direction in 3D) are readjusted according to the fit and are used in the calculation of the system’s transverse decay-path vector , the invariant mass , and the masses of the two subsystems. Following Refs. belle2013 and bes2013 , we select the larger mass combination as a candidate’s mass.
We select events in the range 4.1–4.7 GeV that includes the and excludes fully reconstructed decays of hadrons to final states where and stand for a pion, a kaon, or a proton. We divide the data into two non-overlapping samples: events with a displaced vertex, selected as in Ref. zc1 , and a complementary sample of “primary vertex” events. The criteria for the displaced vertex category are: the vertex of the and the highest track is required to be displaced in the transverse plane from the interaction vertex by at least 5, the significance of the impact parameter in the transverse plane (IP) ip of the leading track is required to be greater than 2, the second track’s IP significance is required to be greater than 1, and the second track’s contribution to the +2 tracks vertex must be less than 6. The cosine of the angle in the transverse plane between the momentum vector and decay path of the tracks system is required to be greater than 0.9.
The sample includes events where the hadronic pair comes from decays K^{*}$$\rightarrow$$K\pi or \phi$$\rightarrow$$KK. We remove such events by assuming that one or both of the charged hadrons are kaons and vetoing the mass combinations GeV and GeV. We also veto photon conversions by removing events with GeV. The decay-length distributions in the transverse plane for events in the “displaced vertex” and the “primary vertex” categories in the mass range GeV are shown in Fig. 1.
III mass fits
We study the system in the vicinity of the . We perform a binned maximum-likelihood fit of the distribution to a sum of a resonant signal and an incoherent background in six intervals of : 4.1–4.2 GeV, 4.2–4.3 GeV, 4.3–4.4 GeV, 4.4–4.5 GeV, 4.5–4.6 GeV, and 4.6–4.7 GeV. The signal is represented by the -wave relativistic Breit-Wigner function convolved with a Gaussian mass resolution. The mass and width are fixed to the values for the channels only (see Ref. zcpdg1 ): MeV, MeV. The D0 mass resolution at this mass is MeV. In these fits we allow negative values for the signal yield.
For the “displaced vertex” selection, background is mainly due to weak decays of hadrons to a paired randomly with hadrons coming from the same multi-body decay. For the “primary vertex” events, the main background is due to a promptly produced combined with particles produced in the hadronization process. In both cases we use Chebyshev polynomials of the first kind to represent background. The fitting range limits are chosen so as to obtain an acceptable fit in a maximum range while avoiding areas where the total probability density function goes to zero. We choose the order of the Chebyshev polynomial to minimize the Akaike information test () aic . For a fit with free parameters to a distribution in bins the is defined as . For the displaced-vertex subsample we choose a 4th-order polynomial, and for the “primary vertex” sample the choice is a 5th-order polynomial.
IV Fit results
The results of the fits are shown in Figs. 2 and 3 and summarized in Table 1 and in Fig. 4. The statistical significance of the signal is defined as , where and are likelihood values at the best-fit signal yield and the signal yield fixed to zero. In the case of a negative signal yield, corresponds to the statisical significance of the depletion.
For the “displaced-vertex” subsample we see a clear enhancement near the mass for events in the range GeV, consistent with coming from the which has a mass of MeV pdg , and a smaller excess in the ranges 4.5–4.6 GeV and 4.6–4.7 GeV. In the mass interval 4.3–4.4 GeV (and to smaller extent for 4.4–4.5 GeV) our fits show a negative, but not significant, yield of events. There is no significant signal in the “primary vertex” subsamples in any interval.
For the “displaced-vertex events” in the mass range GeV we also perform a fit allowing the signal mass and width to vary. From this fit, shown in Fig. 5, we obtain our best measurement of the signal: MeV, MeV. The signal yield is events, the fit quality is , and the statistical significance is .
V Acceptance of the displaced-vertex selection
We obtain the acceptance of the “displaced-vertex” selection for decay events leading to using candidates for the decay , assuming that the distributions of the decay length and its uncertainty for the decay are a good representation for the average hadron. Events are required to satisfy the same kinematic and quality cuts as applied above. We find the fitted numbers of decays and , respectively. The ratios of to for and events with the same topology should be the same, to the extent that the lifetimes of and are the same. With the systematic uncertainty discussed in the next section taken into account, the acceptance of the displaced vertex selection is .
VI Systematic uncertainties
VI.1 Mass and width
We assign an asymmetric systematic uncertainty of MeV to the mass measurement due to a bias in mass measurements of hadrons at D0. We assign the uncertainty on the mass and width due to uncertainty in the mass resolution as half of the difference of the results obtained by changing the resolution by to 15 MeV and 19 MeV. We assign uncertainties due to the background shape based on the differences in the results using the 3rd, 4th, and 5th-order polynomial. The systematic uncertainties are summarized in Table 2.
VI.2 Signal yields
The uncertainty in the relative yields of prompt and nonprompt production of the is dominated by statistical uncertainties. The systematic uncertainties are evaluated as follows.
- •
Mass resolution
We assign the uncertainty in the signal yields due to uncertainty in the mass resolution as half of the difference of the results obtained by changing the resolution by to 15 MeV and 19 MeV.
- •
Trigger bias
Some of the single-muon triggers include a trigger term requiring the presence of tracks with non-zero impact parameter. Events recorded solely by such triggers constitute approximately 5% of all events. We assign a systematic uncertainty of % to due to this effect.
- •
Acceptance of the displaced-vertex selection
Our assumption of the equality of the displaced-vertex selection acceptance for the non-prompt and for is based on expectation of the equality of the average lifetime of -hadron parents of the and that of the . The world-average of the lifetime is 3% lower than the lifetime averaged over all hadron species pdg . This difference corresponds to a 1% difference in the acceptance. In addition, there may be small differences between different channels in the transverse momentum distributions of the parent hadrons and of the final-state particles. When the decay is used to estimate the “displaced-vertex” selection acceptance, the result is . We assign a 2% uncertainty to the displaced-vertex acceptance to account for the differences between the decay and decays.
- •
Signal model
We vary the fixed parameters zcpdg1 of the signal mass and width by 2.7 MeV and 6.5 MeV, respectively, corresponding to 1.
- •
Background shape
For the “displaced vertex” selection, we assign a symmetric uncertainty based on the differences between the results obtained using the 3rd, 4th, and 5th order polynomial. For the “primary vertex” selection, we assign an asymmetric uncertainty equal to the difference in the results using the 5th-order and 4th-order polynomial. The systematic uncertainties in the signal yield are summarized in Table 3.
VII Extracting limits on prompt production rates
Using results of the mass fits to the “displaced-vertex” and “primary vertex” subsamples and the above value of the acceptance of the displaced vertex selection, we can obtain acceptance-corrected yields of prompt and nonprompt production and their ratio. We determine the yield for the mass range 4.2–4.3 GeV where the nonprompt signal is statistically significant.
The mass spectrum in the range 4.2–4.3 GeV in the “primary vertex” category shows no clear signal and a large background of about 500070 events in the signal region. While there is no visible signal, we cannot exclude a yield comparable to the nonprompt signal.
In calculating the prompt-to-nonprompt ratio, we first obtain the total yield of the nonprompt production by dividing by the acceptance . That gives (stat + syst).
Of the above number, a fraction equal to falls into the “primary vertex” category and must be subtracted to obtain the net number of prompt events, . In calculating the uncertainty on the total prompt yield, we add the statistical and the systematic uncertainty components in quadrature. We obtain the ratio . Assuming Gaussian uncertainties and setting the Bayesian prior for negative values of to zero, we obtain an upper limit of 0.70 at the 95% credibility level.
VIII Summary and conclusions
Using the D0 Run II data reconstructed with a dedicated extended-tracking algorithm optimized for low- tracks, we have studied production of the exotic state in the decays of hadrons to a system with a subsequent decay to . The observation is consistent with the sequential decay of a -flavored hadron , , . We find a signal at a statistical significance of 5.4 for events with GeV, and find its mass and width to be MeV and MeV in agreement with world average values pdg ; zcpdg1 .
We searched for evidence of the prompt production of with subsequent rapid decays to . In the absence of a significant signal we set an upper limit at the 95% credibility level on the ratio of prompt to nonprompt production, . This upper limit is significantly lower than that observed for , for which is in the range two to three 7tev3872 ; 8tev3872 , and , for which N_{\rm prompt}/N_{\rm nonprompt}$$\approx 1.5 d04140 .
This document was prepared by the D0 collaboration using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359.
We thank the staffs at Fermilab and collaborating institutions, and acknowledge support from the Department of Energy and National Science Foundation (United States of America); Alternative Energies and Atomic Energy Commission and National Center for Scientific Research/National Institute of Nuclear and Particle Physics (France); Ministry of Education and Science of the Russian Federation, National Research Center “Kurchatov Institute” of the Russian Federation, and Russian Foundation for Basic Research (Russia); National Council for the Development of Science and Technology and Carlos Chagas Filho Foundation for the Support of Research in the State of Rio de Janeiro (Brazil); Department of Atomic Energy and Department of Science and Technology (India); Administrative Department of Science, Technology and Innovation (Colombia); National Council of Science and Technology (Mexico); National Research Foundation of Korea (Korea); Foundation for Fundamental Research on Matter (The Netherlands); Science and Technology Facilities Council and The Royal Society (United Kingdom); Ministry of Education, Youth and Sports (Czech Republic); Bundesministerium für Bildung und Forschung (Federal Ministry of Education and Research) and Deutsche Forschungsgemeinschaft (German Research Foundation) (Germany); Science Foundation Ireland (Ireland); Swedish Research Council (Sweden); China Academy of Sciences and National Natural Science Foundation of China (China); and Ministry of Education and Science of Ukraine (Ukraine).
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