Nuclear-modification factor of charged hadrons at forward and backward rapidity in $p$$+$Al and $p$$+$Au collisions at $\sqrt{s_{_{NN}}}=200$ GeV
C. Aidala, Y. Akiba, M. Alfred, V. Andrieux, N. Apadula, H. Asano, B., Azmoun, V. Babintsev, N.S. Bandara, K.N. Barish, S. Bathe, A. Bazilevsky, M., Beaumier, R. Belmont, A. Berdnikov, Y. Berdnikov, D.S. Blau, J.S. Bok, M.L., Brooks, J. Bryslawskyj, V. Bumazhnov, S. Campbell

TL;DR
This study measures how charged hadron production in proton-nucleus collisions at 200 GeV varies with rapidity and collision centrality, revealing suppression at forward rapidity and enhancement at backward rapidity, with results compared to nuclear parton distribution models.
Contribution
It provides new measurements of nuclear modification factors at forward and backward rapidities in $p$+Al and $p$+Au collisions, highlighting differences in nuclear effects and testing theoretical models.
Findings
Suppression of charged hadrons at forward rapidity in central collisions.
Enhancement of charged hadrons at backward rapidity, larger in $p$+Au than $p$+Al.
Nuclear parton distribution functions agree at forward rapidity but not at backward rapidity.
Abstract
The PHENIX experiment has studied nuclear effects in Al and Au collisions at GeV on charged hadron production at forward rapidity (, -going direction) and backward rapidity (, -going direction). Such effects are quantified by measuring nuclear modification factors as a function of transverse momentum and pseudorapidity in various collision multiplicity selections. In central Al and Au collisions, a suppression (enhancement) is observed at forward (backward) rapidity compared to the binary scaled yields in + collisions. The magnitude of enhancement at backward rapidity is larger in Au collisions than in Al collisions, which have a smaller number of participating nucleons. However, the results at forward rapidity show a similar suppression within uncertainties. The results in the…
| collision system | centrality | bias factor | |
|---|---|---|---|
| Al | 0%–5% | 4.10.4 | 0.750.01 |
| 5%–10% | 3.50.3 | 0.810.01 | |
| 10%–20% | 2.90.3 | 0.840.01 | |
| 20%–40% | 2.40.1 | 0.900.02 | |
| 40%–72% | 1.70.1 | 1.040.04 | |
| 0%–100% | 2.10.1 | 0.800.02 | |
| Au | 0%–5% | 9.70.6 | 0.860.01 |
| 5%–10% | 8.40.6 | 0.900.01 | |
| 10%–20% | 7.40.5 | 0.940.01 | |
| 20%–40% | 6.10.4 | 0.980.01 | |
| 40%–60% | 4.40.3 | 1.030.01 | |
| 60%–84% | 2.60.2 | 1.000.06 | |
| 0%–100% | 4.70.3 | 0.860.01 |
| Collision system | FVTX | MuTr-MuID |
|---|---|---|
| + | 2.8%(S), 2.6%(N) | 4.8%(S), 5.6%(N) |
| Al | 2.4%(S), 2.1%(N) | 3.0%(S), 2.8%(N) |
| Au | 2.7%(S), 2.3%(N) | 7.2%(S), 2.7%(N) |
| Source | Relative uncertainty |
|---|---|
| 9.5–9.9% (+) | |
| Acceptance and efficiency | 9.8–10.7% (Al) |
| 9.8–12.6% (Au) | |
| Secondary hadron | 3% |
| BBC efficiency and centrality bias correction | 10% (+) |
| 1.3–4.2% (Al) | |
| 0.4–1.2% (Au) | |
| 4.7–8.5% (Al) | |
| 5.8–6.6% (Au) |
| parameter | value | description |
|---|---|---|
| SoftQCD:inelastic=on | on | QCD process for MB |
| PDF:pSet | 7 | cteq6l parton distribution function |
| MultipartonInteractions:Kfactor | 0.5 | Multiplication factor for multiparton interaction |
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PHENIX Collaboration
Nuclear-modification factor of charged hadrons at forward and
backward rapidity in p$$+Al and p$$+Au collisions at GeV
C. Aidala
Department of Physics, University of Michigan, Ann Arbor, Michigan 48109-1040, USA
Y. Akiba
RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan
RIKEN BNL Research Center, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
M. Alfred
Department of Physics and Astronomy, Howard University, Washington, DC 20059, USA
V. Andrieux
Department of Physics, University of Michigan, Ann Arbor, Michigan 48109-1040, USA
N. Apadula
Iowa State University, Ames, Iowa 50011, USA
H. Asano
Kyoto University, Kyoto 606-8502, Japan
RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan
B. Azmoun
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
V. Babintsev
IHEP Protvino, State Research Center of Russian Federation, Institute for High Energy Physics, Protvino, 142281, Russia
N.S. Bandara
Department of Physics, University of Massachusetts, Amherst, Massachusetts 01003-9337, USA
K.N. Barish
University of California-Riverside, Riverside, California 92521, USA
S. Bathe
Baruch College, City University of New York, New York, New York, 10010 USA
RIKEN BNL Research Center, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
A. Bazilevsky
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
M. Beaumier
University of California-Riverside, Riverside, California 92521, USA
R. Belmont
University of Colorado, Boulder, Colorado 80309, USA
Physics and Astronomy Department, University of North Carolina at Greensboro, Greensboro, North Carolina 27412, USA
A. Berdnikov
Saint Petersburg State Polytechnic University, St. Petersburg, 195251 Russia
Y. Berdnikov
Saint Petersburg State Polytechnic University, St. Petersburg, 195251 Russia
D.S. Blau
National Research Center “Kurchatov Institute”, Moscow, 123098 Russia
National Research Nuclear University, MEPhI, Moscow Engineering Physics Institute, Moscow, 115409, Russia
J.S. Bok
New Mexico State University, Las Cruces, New Mexico 88003, USA
M.L. Brooks
Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
J. Bryslawskyj
Baruch College, City University of New York, New York, New York, 10010 USA
University of California-Riverside, Riverside, California 92521, USA
V. Bumazhnov
IHEP Protvino, State Research Center of Russian Federation, Institute for High Energy Physics, Protvino, 142281, Russia
S. Campbell
Columbia University, New York, New York 10027 and Nevis Laboratories, Irvington, New York 10533, USA
V. Canoa Roman
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
R. Cervantes
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
C.Y. Chi
Columbia University, New York, New York 10027 and Nevis Laboratories, Irvington, New York 10533, USA
M. Chiu
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
I.J. Choi
University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA
J.B. Choi
Deceased
Jeonbuk National University, Jeonju, 54896, Korea
Z. Citron
Weizmann Institute, Rehovot 76100, Israel
M. Connors
Georgia State University, Atlanta, Georgia 30303, USA
RIKEN BNL Research Center, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
N. Cronin
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
M. Csanád
ELTE, Eötvös Loránd University, H-1117 Budapest, Pázmány P. s. 1/A, Hungary
T. Csörgő
Eszterházy Károly University, Károly Róbert Campus, H-3200 Gyöngyös, Mátrai út 36, Hungary
Institute for Particle and Nuclear Physics, Wigner Research Centre for Physics, Hungarian Academy of Sciences (Wigner RCP, RMKI) H-1525 Budapest 114, POBox 49, Budapest, Hungary
T.W. Danley
Department of Physics and Astronomy, Ohio University, Athens, Ohio 45701, USA
M.S. Daugherity
Abilene Christian University, Abilene, Texas 79699, USA
G. David
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
Debrecen University, H-4010 Debrecen, Egyetem tér 1, Hungary
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
K. DeBlasio
University of New Mexico, Albuquerque, New Mexico 87131, USA
K. Dehmelt
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
A. Denisov
IHEP Protvino, State Research Center of Russian Federation, Institute for High Energy Physics, Protvino, 142281, Russia
A. Deshpande
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
RIKEN BNL Research Center, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
E.J. Desmond
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
A. Dion
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
D. Dixit
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
J.H. Do
Yonsei University, IPAP, Seoul 120-749, Korea
A. Drees
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
K.A. Drees
Collider-Accelerator Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
J.M. Durham
Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
A. Durum
IHEP Protvino, State Research Center of Russian Federation, Institute for High Energy Physics, Protvino, 142281, Russia
A. Enokizono
RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan
Physics Department, Rikkyo University, 3-34-1 Nishi-Ikebukuro, Toshima, Tokyo 171-8501, Japan
H. En’yo
RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan
S. Esumi
Tomonaga Center for the History of the Universe, University of Tsukuba, Tsukuba, Ibaraki 305, Japan
B. Fadem
Muhlenberg College, Allentown, Pennsylvania 18104-5586, USA
W. Fan
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
N. Feege
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
D.E. Fields
University of New Mexico, Albuquerque, New Mexico 87131, USA
M. Finger
Charles University, Ovocný trh 5, Praha 1, 116 36, Prague, Czech Republic
M. Finger, Jr
Charles University, Ovocný trh 5, Praha 1, 116 36, Prague, Czech Republic
S.L. Fokin
National Research Center “Kurchatov Institute”, Moscow, 123098 Russia
J.E. Frantz
Department of Physics and Astronomy, Ohio University, Athens, Ohio 45701, USA
A. Franz
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
A.D. Frawley
Florida State University, Tallahassee, Florida 32306, USA
Y. Fukuda
Tomonaga Center for the History of the Universe, University of Tsukuba, Tsukuba, Ibaraki 305, Japan
C. Gal
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
P. Gallus
Czech Technical University, Zikova 4, 166 36 Prague 6, Czech Republic
E.A. Gamez
Department of Physics, University of Michigan, Ann Arbor, Michigan 48109-1040, USA
P. Garg
Department of Physics, Banaras Hindu University, Varanasi 221005, India
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
H. Ge
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
F. Giordano
University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA
Y. Goto
RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan
RIKEN BNL Research Center, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
N. Grau
Department of Physics, Augustana University, Sioux Falls, South Dakota 57197, USA
S.V. Greene
Vanderbilt University, Nashville, Tennessee 37235, USA
M. Grosse Perdekamp
University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA
T. Gunji
Center for Nuclear Study, Graduate School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033, Japan
H. Guragain
Georgia State University, Atlanta, Georgia 30303, USA
T. Hachiya
Nara Women’s University, Kita-uoya Nishi-machi Nara 630-8506, Japan
RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan
RIKEN BNL Research Center, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
J.S. Haggerty
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
K.I. Hahn
Ewha Womans University, Seoul 120-750, Korea
H. Hamagaki
Center for Nuclear Study, Graduate School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033, Japan
H.F. Hamilton
Abilene Christian University, Abilene, Texas 79699, USA
S.Y. Han
Ewha Womans University, Seoul 120-750, Korea
RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan
J. Hanks
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
S. Hasegawa
Advanced Science Research Center, Japan Atomic Energy Agency, 2-4 Shirakata Shirane, Tokai-mura, Naka-gun, Ibaraki-ken 319-1195, Japan
T.O.S. Haseler
Georgia State University, Atlanta, Georgia 30303, USA
X. He
Georgia State University, Atlanta, Georgia 30303, USA
T.K. Hemmick
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
J.C. Hill
Iowa State University, Ames, Iowa 50011, USA
K. Hill
University of Colorado, Boulder, Colorado 80309, USA
A. Hodges
Georgia State University, Atlanta, Georgia 30303, USA
R.S. Hollis
University of California-Riverside, Riverside, California 92521, USA
K. Homma
Hiroshima University, Kagamiyama, Higashi-Hiroshima 739-8526, Japan
B. Hong
Korea University, Seoul, 02841
T. Hoshino
Hiroshima University, Kagamiyama, Higashi-Hiroshima 739-8526, Japan
N. Hotvedt
Iowa State University, Ames, Iowa 50011, USA
J. Huang
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
S. Huang
Vanderbilt University, Nashville, Tennessee 37235, USA
K. Imai
Advanced Science Research Center, Japan Atomic Energy Agency, 2-4 Shirakata Shirane, Tokai-mura, Naka-gun, Ibaraki-ken 319-1195, Japan
M. Inaba
Tomonaga Center for the History of the Universe, University of Tsukuba, Tsukuba, Ibaraki 305, Japan
A. Iordanova
University of California-Riverside, Riverside, California 92521, USA
D. Isenhower
Abilene Christian University, Abilene, Texas 79699, USA
S. Ishimaru
Nara Women’s University, Kita-uoya Nishi-machi Nara 630-8506, Japan
D. Ivanishchev
PNPI, Petersburg Nuclear Physics Institute, Gatchina, Leningrad region, 188300, Russia
B.V. Jacak
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
M. Jezghani
Georgia State University, Atlanta, Georgia 30303, USA
Z. Ji
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
X. Jiang
Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
B.M. Johnson
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
Georgia State University, Atlanta, Georgia 30303, USA
D. Jouan
IPN-Orsay, Univ. Paris-Sud, CNRS/IN2P3, Université Paris-Saclay, BP1, F-91406, Orsay, France
D.S. Jumper
University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA
J.H. Kang
Yonsei University, IPAP, Seoul 120-749, Korea
D. Kapukchyan
University of California-Riverside, Riverside, California 92521, USA
S. Karthas
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
D. Kawall
Department of Physics, University of Massachusetts, Amherst, Massachusetts 01003-9337, USA
A.V. Kazantsev
National Research Center “Kurchatov Institute”, Moscow, 123098 Russia
V. Khachatryan
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
A. Khanzadeev
PNPI, Petersburg Nuclear Physics Institute, Gatchina, Leningrad region, 188300, Russia
A. Khatiwada
Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
C. Kim
University of California-Riverside, Riverside, California 92521, USA
Korea University, Seoul, 02841
E.-J. Kim
Jeonbuk National University, Jeonju, 54896, Korea
M. Kim
RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan
Department of Physics and Astronomy, Seoul National University, Seoul 151-742, Korea
D. Kincses
ELTE, Eötvös Loránd University, H-1117 Budapest, Pázmány P. s. 1/A, Hungary
E. Kistenev
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
J. Klatsky
Florida State University, Tallahassee, Florida 32306, USA
P. Kline
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
T. Koblesky
University of Colorado, Boulder, Colorado 80309, USA
D. Kotov
PNPI, Petersburg Nuclear Physics Institute, Gatchina, Leningrad region, 188300, Russia
Saint Petersburg State Polytechnic University, St. Petersburg, 195251 Russia
S. Kudo
Tomonaga Center for the History of the Universe, University of Tsukuba, Tsukuba, Ibaraki 305, Japan
B. Kurgyis
ELTE, Eötvös Loránd University, H-1117 Budapest, Pázmány P. s. 1/A, Hungary
K. Kurita
Physics Department, Rikkyo University, 3-34-1 Nishi-Ikebukuro, Toshima, Tokyo 171-8501, Japan
Y. Kwon
Yonsei University, IPAP, Seoul 120-749, Korea
J.G. Lajoie
Iowa State University, Ames, Iowa 50011, USA
A. Lebedev
Iowa State University, Ames, Iowa 50011, USA
S. Lee
Yonsei University, IPAP, Seoul 120-749, Korea
S.H. Lee
Iowa State University, Ames, Iowa 50011, USA
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
M.J. Leitch
Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
Y.H. Leung
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
N.A. Lewis
Department of Physics, University of Michigan, Ann Arbor, Michigan 48109-1040, USA
X. Li
Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
S.H. Lim
Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
Yonsei University, IPAP, Seoul 120-749, Korea
M.X. Liu
Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
V.-R. Loggins
University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA
S. Lökös
ELTE, Eötvös Loránd University, H-1117 Budapest, Pázmány P. s. 1/A, Hungary
Eszterházy Károly University, Károly Róbert Campus, H-3200 Gyöngyös, Mátrai út 36, Hungary
K. Lovasz
Debrecen University, H-4010 Debrecen, Egyetem tér 1, Hungary
D. Lynch
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
T. Majoros
Debrecen University, H-4010 Debrecen, Egyetem tér 1, Hungary
Y.I. Makdisi
Collider-Accelerator Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
M. Makek
Department of Physics, Faculty of Science, University of Zagreb, Bijenička c. 32 HR-10002 Zagreb, Croatia
V.I. Manko
National Research Center “Kurchatov Institute”, Moscow, 123098 Russia
E. Mannel
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
M. McCumber
Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
P.L. McGaughey
Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
D. McGlinchey
University of Colorado, Boulder, Colorado 80309, USA
Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
C. McKinney
University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA
M. Mendoza
University of California-Riverside, Riverside, California 92521, USA
W.J. Metzger
Eszterházy Károly University, Károly Róbert Campus, H-3200 Gyöngyös, Mátrai út 36, Hungary
A.C. Mignerey
University of Maryland, College Park, Maryland 20742, USA
A. Milov
Weizmann Institute, Rehovot 76100, Israel
D.K. Mishra
Bhabha Atomic Research Centre, Bombay 400 085, India
J.T. Mitchell
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
Iu. Mitrankov
Saint Petersburg State Polytechnic University, St. Petersburg, 195251 Russia
G. Mitsuka
KEK, High Energy Accelerator Research Organization, Tsukuba, Ibaraki 305-0801, Japan
RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan
RIKEN BNL Research Center, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
S. Miyasaka
RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan
Department of Physics, Tokyo Institute of Technology, Oh-okayama, Meguro, Tokyo 152-8551, Japan
S. Mizuno
RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan
Tomonaga Center for the History of the Universe, University of Tsukuba, Tsukuba, Ibaraki 305, Japan
P. Montuenga
University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA
T. Moon
Yonsei University, IPAP, Seoul 120-749, Korea
D.P. Morrison
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
S.I. Morrow
Vanderbilt University, Nashville, Tennessee 37235, USA
T. Murakami
Kyoto University, Kyoto 606-8502, Japan
RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan
J. Murata
RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan
Physics Department, Rikkyo University, 3-34-1 Nishi-Ikebukuro, Toshima, Tokyo 171-8501, Japan
K. Nagai
Department of Physics, Tokyo Institute of Technology, Oh-okayama, Meguro, Tokyo 152-8551, Japan
K. Nagashima
Hiroshima University, Kagamiyama, Higashi-Hiroshima 739-8526, Japan
RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan
T. Nagashima
Physics Department, Rikkyo University, 3-34-1 Nishi-Ikebukuro, Toshima, Tokyo 171-8501, Japan
J.L. Nagle
University of Colorado, Boulder, Colorado 80309, USA
M.I. Nagy
ELTE, Eötvös Loránd University, H-1117 Budapest, Pázmány P. s. 1/A, Hungary
I. Nakagawa
RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan
RIKEN BNL Research Center, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
K. Nakano
RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan
Department of Physics, Tokyo Institute of Technology, Oh-okayama, Meguro, Tokyo 152-8551, Japan
C. Nattrass
University of Tennessee, Knoxville, Tennessee 37996, USA
S. Nelson
Florida A&M University, Tallahassee, FL 32307, USA
T. Niida
Tomonaga Center for the History of the Universe, University of Tsukuba, Tsukuba, Ibaraki 305, Japan
R. Nishitani
Nara Women’s University, Kita-uoya Nishi-machi Nara 630-8506, Japan
R. Nouicer
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
RIKEN BNL Research Center, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
T. Novák
Eszterházy Károly University, Károly Róbert Campus, H-3200 Gyöngyös, Mátrai út 36, Hungary
Institute for Particle and Nuclear Physics, Wigner Research Centre for Physics, Hungarian Academy of Sciences (Wigner RCP, RMKI) H-1525 Budapest 114, POBox 49, Budapest, Hungary
N. Novitzky
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
A.S. Nyanin
National Research Center “Kurchatov Institute”, Moscow, 123098 Russia
E. O’Brien
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
C.A. Ogilvie
Iowa State University, Ames, Iowa 50011, USA
J.D. Orjuela Koop
University of Colorado, Boulder, Colorado 80309, USA
J.D. Osborn
Department of Physics, University of Michigan, Ann Arbor, Michigan 48109-1040, USA
A. Oskarsson
Department of Physics, Lund University, Box 118, SE-221 00 Lund, Sweden
G.J. Ottino
University of New Mexico, Albuquerque, New Mexico 87131, USA
K. Ozawa
KEK, High Energy Accelerator Research Organization, Tsukuba, Ibaraki 305-0801, Japan
Tomonaga Center for the History of the Universe, University of Tsukuba, Tsukuba, Ibaraki 305, Japan
V. Pantuev
Institute for Nuclear Research of the Russian Academy of Sciences, prospekt 60-letiya Oktyabrya 7a, Moscow 117312, Russia
V. Papavassiliou
New Mexico State University, Las Cruces, New Mexico 88003, USA
J.S. Park
Department of Physics and Astronomy, Seoul National University, Seoul 151-742, Korea
S. Park
RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan
Department of Physics and Astronomy, Seoul National University, Seoul 151-742, Korea
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
S.F. Pate
New Mexico State University, Las Cruces, New Mexico 88003, USA
M. Patel
Iowa State University, Ames, Iowa 50011, USA
W. Peng
Vanderbilt University, Nashville, Tennessee 37235, USA
D.V. Perepelitsa
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
University of Colorado, Boulder, Colorado 80309, USA
G.D.N. Perera
New Mexico State University, Las Cruces, New Mexico 88003, USA
D.Yu. Peressounko
National Research Center “Kurchatov Institute”, Moscow, 123098 Russia
C.E. PerezLara
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
J. Perry
Iowa State University, Ames, Iowa 50011, USA
R. Petti
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
M. Phipps
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA
C. Pinkenburg
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
R.P. Pisani
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
A. Pun
Department of Physics and Astronomy, Ohio University, Athens, Ohio 45701, USA
M.L. Purschke
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
P.V. Radzevich
Saint Petersburg State Polytechnic University, St. Petersburg, 195251 Russia
K.F. Read
Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
University of Tennessee, Knoxville, Tennessee 37996, USA
D. Reynolds
Chemistry Department, Stony Brook University, SUNY, Stony Brook, New York 11794-3400, USA
V. Riabov
National Research Nuclear University, MEPhI, Moscow Engineering Physics Institute, Moscow, 115409, Russia
PNPI, Petersburg Nuclear Physics Institute, Gatchina, Leningrad region, 188300, Russia
Y. Riabov
PNPI, Petersburg Nuclear Physics Institute, Gatchina, Leningrad region, 188300, Russia
Saint Petersburg State Polytechnic University, St. Petersburg, 195251 Russia
D. Richford
Baruch College, City University of New York, New York, New York, 10010 USA
T. Rinn
Iowa State University, Ames, Iowa 50011, USA
S.D. Rolnick
University of California-Riverside, Riverside, California 92521, USA
M. Rosati
Iowa State University, Ames, Iowa 50011, USA
Z. Rowan
Baruch College, City University of New York, New York, New York, 10010 USA
J. Runchey
Iowa State University, Ames, Iowa 50011, USA
A.S. Safonov
Saint Petersburg State Polytechnic University, St. Petersburg, 195251 Russia
T. Sakaguchi
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
H. Sako
Advanced Science Research Center, Japan Atomic Energy Agency, 2-4 Shirakata Shirane, Tokai-mura, Naka-gun, Ibaraki-ken 319-1195, Japan
V. Samsonov
National Research Nuclear University, MEPhI, Moscow Engineering Physics Institute, Moscow, 115409, Russia
PNPI, Petersburg Nuclear Physics Institute, Gatchina, Leningrad region, 188300, Russia
M. Sarsour
Georgia State University, Atlanta, Georgia 30303, USA
S. Sato
Advanced Science Research Center, Japan Atomic Energy Agency, 2-4 Shirakata Shirane, Tokai-mura, Naka-gun, Ibaraki-ken 319-1195, Japan
C.Y. Scarlett
Florida A&M University, Tallahassee, FL 32307, USA
B. Schaefer
Vanderbilt University, Nashville, Tennessee 37235, USA
B.K. Schmoll
University of Tennessee, Knoxville, Tennessee 37996, USA
K. Sedgwick
University of California-Riverside, Riverside, California 92521, USA
R. Seidl
RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan
RIKEN BNL Research Center, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
A. Sen
Iowa State University, Ames, Iowa 50011, USA
University of Tennessee, Knoxville, Tennessee 37996, USA
R. Seto
University of California-Riverside, Riverside, California 92521, USA
A. Sexton
University of Maryland, College Park, Maryland 20742, USA
D. Sharma
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
I. Shein
IHEP Protvino, State Research Center of Russian Federation, Institute for High Energy Physics, Protvino, 142281, Russia
T.-A. Shibata
RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan
Department of Physics, Tokyo Institute of Technology, Oh-okayama, Meguro, Tokyo 152-8551, Japan
K. Shigaki
Hiroshima University, Kagamiyama, Higashi-Hiroshima 739-8526, Japan
M. Shimomura
Iowa State University, Ames, Iowa 50011, USA
Nara Women’s University, Kita-uoya Nishi-machi Nara 630-8506, Japan
T. Shioya
Tomonaga Center for the History of the Universe, University of Tsukuba, Tsukuba, Ibaraki 305, Japan
P. Shukla
Bhabha Atomic Research Centre, Bombay 400 085, India
A. Sickles
University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA
C.L. Silva
Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
D. Silvermyr
Department of Physics, Lund University, Box 118, SE-221 00 Lund, Sweden
B.K. Singh
Department of Physics, Banaras Hindu University, Varanasi 221005, India
C.P. Singh
Department of Physics, Banaras Hindu University, Varanasi 221005, India
V. Singh
Department of Physics, Banaras Hindu University, Varanasi 221005, India
M.J. Skoby
Department of Physics, University of Michigan, Ann Arbor, Michigan 48109-1040, USA
M. Slunečka
Charles University, Ovocný trh 5, Praha 1, 116 36, Prague, Czech Republic
K.L. Smith
Florida State University, Tallahassee, Florida 32306, USA
M. Snowball
Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
R.A. Soltz
Lawrence Livermore National Laboratory, Livermore, California 94550, USA
W.E. Sondheim
Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
S.P. Sorensen
University of Tennessee, Knoxville, Tennessee 37996, USA
I.V. Sourikova
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
P.W. Stankus
Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
S.P. Stoll
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
T. Sugitate
Hiroshima University, Kagamiyama, Higashi-Hiroshima 739-8526, Japan
A. Sukhanov
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
T. Sumita
RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan
J. Sun
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
Z. Sun
Debrecen University, H-4010 Debrecen, Egyetem tér 1, Hungary
S. Suzuki
Nara Women’s University, Kita-uoya Nishi-machi Nara 630-8506, Japan
J. Sziklai
Institute for Particle and Nuclear Physics, Wigner Research Centre for Physics, Hungarian Academy of Sciences (Wigner RCP, RMKI) H-1525 Budapest 114, POBox 49, Budapest, Hungary
K. Tanida
Advanced Science Research Center, Japan Atomic Energy Agency, 2-4 Shirakata Shirane, Tokai-mura, Naka-gun, Ibaraki-ken 319-1195, Japan
RIKEN BNL Research Center, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
Department of Physics and Astronomy, Seoul National University, Seoul 151-742, Korea
M.J. Tannenbaum
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
S. Tarafdar
Vanderbilt University, Nashville, Tennessee 37235, USA
Weizmann Institute, Rehovot 76100, Israel
A. Taranenko
National Research Nuclear University, MEPhI, Moscow Engineering Physics Institute, Moscow, 115409, Russia
G. Tarnai
Debrecen University, H-4010 Debrecen, Egyetem tér 1, Hungary
R. Tieulent
Georgia State University, Atlanta, Georgia 30303, USA
IPNL, CNRS/IN2P3, Univ Lyon, Université Lyon 1, F-69622, Villeurbanne, France
A. Timilsina
Iowa State University, Ames, Iowa 50011, USA
T. Todoroki
RIKEN BNL Research Center, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
Tomonaga Center for the History of the Universe, University of Tsukuba, Tsukuba, Ibaraki 305, Japan
M. Tomášek
Czech Technical University, Zikova 4, 166 36 Prague 6, Czech Republic
C.L. Towell
Abilene Christian University, Abilene, Texas 79699, USA
R.S. Towell
Abilene Christian University, Abilene, Texas 79699, USA
I. Tserruya
Weizmann Institute, Rehovot 76100, Israel
Y. Ueda
Hiroshima University, Kagamiyama, Higashi-Hiroshima 739-8526, Japan
B. Ujvari
Debrecen University, H-4010 Debrecen, Egyetem tér 1, Hungary
H.W. van Hecke
Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
J. Velkovska
Vanderbilt University, Nashville, Tennessee 37235, USA
M. Virius
Czech Technical University, Zikova 4, 166 36 Prague 6, Czech Republic
V. Vrba
Czech Technical University, Zikova 4, 166 36 Prague 6, Czech Republic
Institute of Physics, Academy of Sciences of the Czech Republic, Na Slovance 2, 182 21 Prague 8, Czech Republic
N. Vukman
Department of Physics, Faculty of Science, University of Zagreb, Bijenička c. 32 HR-10002 Zagreb, Croatia
X.R. Wang
New Mexico State University, Las Cruces, New Mexico 88003, USA
RIKEN BNL Research Center, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
Z. Wang
Baruch College, City University of New York, New York, New York, 10010 USA
Y.S. Watanabe
Center for Nuclear Study, Graduate School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033, Japan
C.P. Wong
Georgia State University, Atlanta, Georgia 30303, USA
C.L. Woody
Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
C. Xu
New Mexico State University, Las Cruces, New Mexico 88003, USA
Q. Xu
Vanderbilt University, Nashville, Tennessee 37235, USA
L. Xue
Georgia State University, Atlanta, Georgia 30303, USA
S. Yalcin
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
Y.L. Yamaguchi
RIKEN BNL Research Center, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
H. Yamamoto
Tomonaga Center for the History of the Universe, University of Tsukuba, Tsukuba, Ibaraki 305, Japan
A. Yanovich
IHEP Protvino, State Research Center of Russian Federation, Institute for High Energy Physics, Protvino, 142281, Russia
J.H. Yoo
Korea University, Seoul, 02841
RIKEN BNL Research Center, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
I. Yoon
Department of Physics and Astronomy, Seoul National University, Seoul 151-742, Korea
H. Yu
New Mexico State University, Las Cruces, New Mexico 88003, USA
Peking University, Beijing 100871, People’s Republic of China
I.E. Yushmanov
National Research Center “Kurchatov Institute”, Moscow, 123098 Russia
W.A. Zajc
Columbia University, New York, New York 10027 and Nevis Laboratories, Irvington, New York 10533, USA
A. Zelenski
Collider-Accelerator Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
Y. Zhai
Iowa State University, Ames, Iowa 50011, USA
S. Zharko
Saint Petersburg State Polytechnic University, St. Petersburg, 195251 Russia
L. Zou
University of California-Riverside, Riverside, California 92521, USA
Abstract
The PHENIX experiment has studied nuclear effects in p$$+Al and p$$+Au collisions at GeV on charged hadron production at forward rapidity (, -going direction) and backward rapidity (, -going direction). Such effects are quantified by measuring nuclear modification factors as a function of transverse momentum and pseudorapidity in various collision multiplicity selections. In central p$$+Al and p$$+Au collisions, a suppression (enhancement) is observed at forward (backward) rapidity compared to the binary scaled yields in + collisions. The magnitude of enhancement at backward rapidity is larger in p$$+Au collisions than in p$$+Al collisions, which have a smaller number of participating nucleons. However, the results at forward rapidity show a similar suppression within uncertainties. The results in the integrated centrality are compared with calculations using nuclear parton distribution functions, which show a reasonable agreement at the forward rapidity but fail to describe the backward rapidity enhancement.
I Introduction
Measurements of particle production in heavy-ion collisions enable the study of properties of a hot and dense nuclear medium called the quark-gluon plasma (QGP) [1, 2, 3, 4]. An initial striking observation at the Relativistic Heavy Ion Collider (RHIC) was that production of high transverse momentum () hadrons in AuAu collisions is strongly suppressed compared to that in + collisions scaled by the number of binary collisions. This suppression indicates that partons experience substantial energy loss as they traverse the QGP, a phenomenon called jet-quenching [5]. A control experiment involving a deuteron projectile on a heavy-ion target, d$$+Au, was carried out to test whether the feature of strong energy loss is still present in a collision system of much smaller size. The results in d$$+Au collisions at midrapidity presented in Ref. [6] showed no suppression at high , initially leading to the conclusion that QGP itself—and associated jet quenching—were unique to collisions of larger heavy ions. In the ten years because these initial measurements, indications of QGP formation in smaller collision systems including d$$+Au have been found, though without evidence of jet quenching phenomena [7].
Although there were no indications of strong suppression of high particles in d$$+Au collisions, detailed measurements do indicate other particle-production modifications relative to + collisions [8, 9, 10, 11, 12]. At midrapidity, a centrality-dependent enhancement of charged hadron production was observed at intermediate (2<\mbox{p_{T}}<5~{}{\rm GeV}/c) [11] in d$$+Au collisions at GeV. These nuclear effects may be due to initial- and/or final-state multiple scatterings of incoming and outgoing partons [13, 14]. Processes such as radial flow [15] and recombination [16] developed for heavy-ion collisions were also investigated to explain a stronger enhancement of and over and [11]. Recent results of collectivity amongst identified particles in small collision systems at RHIC and the Large Hadron Collider [7] have been also explained within the hydrodynamic evolution model [17, 18].
The study of particle production at forward and backward rapidity can provide additional information on nuclear effects such as initial-state energy loss [19] and modification of nuclear parton distribution functions (nPDF) [20, 21, 22, 23, 24]. Of particular interest are gluons at small Bjorken (fraction of the proton’s longitudinal momentum carried by the parton), where the dramatic increase of gluon density leads to expectation of saturation. This is often described within the color glass condensate (CGC) framework [25]. A strong centrality dependent suppression of single and dihadron production has been observed at forward rapidity in d$$+Au collisions at GeV [8, 9, 10]. A CGC calculation provides a good description of the experimental data [26, 27]. Also, a perturbative quantum chromodynamics (pQCD) calculation considering coherent multiple scattering with small- gluons reproduces the suppression of particle production at forward rapidity [19, 28]. Another very different explanation for the suppression at forward rapidity is that color fluctuation effects modify the size of the high- partons in the proton [29, 30].
Accessible quark and gluon ranges depend on the pseudorapidity () and transverse momentum of final state hadrons or jets. Therefore, measurements over a wide kinematic range are quite useful to further understand nuclear effects in small collision systems. PHENIX experiment has two muon spectrometers that provide wide coverage at forward (\mbox{x_{\rm Bj}}\approx 0.02, shadowing region) and backward rapidity (\mbox{x_{\rm Bj}}\approx 0.1, anti-shadowing region). In the previous study of nuclear effects on charged hadron production in d$$+Au collisions at GeV [31], a significant suppression was observed at forward rapidity in high multiplicity collisions compared to that in low multiplicity collisions, whereas a moderate enhancement is seen at backward rapidity. Although the direction of modification is consistent with the expectation from nPDF modification, no specific model comparison was presented.
High statistics data samples of +, p$$+Al, and p$$+Au collisions at GeV were collected in 2015 by PHENIX. These data samples combined with the availability of a new forward silicon vertex tracking detectors, which enable the selection of particle tracks coming from the collision point, significantly improved and resolutions. The charged hadron analysis with these data sets can extend the previous study in d$$+Au collisions [31], and a comparison between p$$+Al and p$$+Au of very different size of nuclei can provide new information on nuclear effects on charged hadron production in p$$+$$A collisions.
In this paper, we present nuclear modification factors of charged hadron production at forward and backward rapidity in p$$+Al and p$$+Au collisions at GeV of various multiplicities. Section II describes the experimental setup and the data sets used in this analysis. Section III details the analysis methods. Section IV discusses systematic uncertainties. Section V presents results and discussion. Section VI gives the summary and conclusions.
II Experimental Setup
The PHENIX detector [32] comprises two central arm spectrometers at midrapidity and two muon arm spectrometers at forward and backward rapidity. The detector configuration during the data taking in 2015 is shown in Fig. 1. The muon spectrometers have full-azimuthal acceptance, covering (south arm) and (north arm). Each muon arm comprises a forward silicon vertex tracker (FVTX), followed by a hadron absorber and a muon spectrometer. The muon spectrometer is composed of a muon tracker (MuTr) embedded in a magnetic field followed by a muon identifier (MuID).
The FVTX is a silicon detector with four stations in each arm. Each station comprises 96 sensors along the direction. Each silicon sensor is finely segmented along the radial direction, with a strip pitch of . The primary purpose of the FVTX is to measure a precise collision vertex also constrained by the silicon vertex tracker (VTX) at midrapidity. The FVTX was also designed to measure precise momentum vector information of charged particles entering the muon spectrometer before suffering large multiple scattering in the hadron absorber. More technical details on the FVTX are available in Ref. [33]. Following the FVTX is the hadron absorber, composed of layers of copper, iron, and stainless steel, corresponding to 7.2 nuclear interaction lengths (). Hadrons entering the absorber are suppressed by a factor of approximately 1000, thus significantly reducing hadronic background for muon-based measurements.
The MuTr has two arms each consisting of three stations of cathode strip chambers, which are inside a magnet with a radial field integral of . The MuTr provides a momentum measurement for charged particles. The MuID is composed of five layers (referred to as gap 0–4) of steel absorber (4.8 (5.4) for south (north) arm) and two planes of Iarocci tubes. This enables the separation of muons and hadrons based on their penetration depth at a given reconstructed momentum. The MuTr and MuID are also used to trigger events containing at least one muon or hadron candidate. The MuID trigger is designed to enrich events with muons by requiring at least one hit in either gap 3 or 4. Hadrons that stop only after partially penetrating the MuID can be enhanced by requiring no hit in gap 4. The MuTr trigger is used to sample high momentum tracks by requiring a track sagitta less than three MuTr cathode strips wide at the middle station of the MuTr. A more detailed discussion of the PHENIX muon arms can be found in Ref. [34, 35].
The beam-beam counters (BBC) [36] comprise two arrays of 64 quartz Čerenkov detectors located at from the nominal interaction point. Each BBC has an acceptance covering the full azimuth and . The BBCs are used to determine the collision-vertex position along the beam axis () with a resolution of roughly 2 cm in + collisions. They also provide a minimum bias (MB) trigger by requiring at least one hit in each BBC. The BBC trigger efficiency, determined from the Van der Meer scan technique [37], is 55% for inelastic + events and 79% for events with midrapidity particle production [38]. In p$$+Al and p$$+Au collisions, charged particle multiplicity in BBC in the Al- and Au-going direction () is used to categorize the event centrality. The BBC trigger is for 72% (84%) of inelastic p$$+Al (p$$+Au) collisions. Centrality dependent bias factors to account for the efficiency for MB triggered events and hard scattering events have been obtained based on the method developed in Ref. [39].
III Data analysis
III.1 Data set
Data sets used in this analysis include +, p$$+Al, and p$$+Au collisions at GeV collected with the PHENIX detector in 2015. Events are required to have |\mbox{z_{\rm BBC}}|<20 cm. The improved precision vertex from the silicon trackers (VTX and FVTX) is not used in this analysis due to the track multiplicity-dependent vertex reconstruction efficiency. The analyzed event samples are required to have at least one track candidate in the MuTr and MuID satisfying either single hadron or single muon trigger in coincidence with the MB trigger. The integrated luminosity of the data used in this analysis is in +, 260 in p$$+Al, and 80 in p$$+Au collisions.
III.2 Hadron selection
The majority of hadrons emitted from the collision are stopped inside the hadron absorber. Hadrons which pass through the hadron absorber enter the MuTr and can still be stopped in the middle of the MuID by producing hadronic showers in the additional steel absorber planes. Low momentum muons can also be stopped due to ionization energy loss, but the momentum distribution measured in the MuTr is very different for these muons and hadrons which are stopped in the MuID. Figure 2 shows the longitudinal momentum () distributions of reconstructed tracks at the north arm MuID gaps 2 and 3 from a full geant4 detector simulation of charged hadrons (see Sec. III.4). Muon tracks from light hadron decays show a narrow distribution in 2.5<\mbox{p_{z}}<3.0~{}{\rm GeV}/c, whereas tracks from hadrons show a much broader distribution. Therefore, tracks from hadrons can be enriched with a proper cut ( for gap 2 and for gap 3). The inset plots show the hadron fraction as a function of with the cuts. The hadron purity is () at MuID gap 2 (gap 3) for \mbox{p_{T}}>1.5~{}{\rm GeV}/c. The contamination of muons in the combined sample for both MuID gap 2 and gap 3 is less than 5% based on this simulation study.
One benefit from the FVTX is that the initial momentum vector of hadrons can be measured precisely before they undergo significant multiple scattering inside the absorber. In particular, the FVTX has very fine segmentation in the radial direction which can improve the and resolution of measured tracks, both of which are important for this analysis. Figure 3 shows the distribution between reconstructed tracks () and true tracks () as a function of for hadron candidates from the geant4 simulation. In the case where momentum information from only the MuTr is used, shown in Fig. 3 (a), the smearing in is quite large. This is significantly improved by requiring association with FVTX tracks, shown in Fig. 3 (b).
III.3 Trigger efficiency
One consideration with the FVTX association requirement is the possibility of multiple FVTX tracks within the search window of a projected MuTr track, due to the higher FVTX track multiplicity and the smeared momentum information from the MuTr as shown in Fig. 3 (a). In this case, a MuTr track can be associated with a wrong FVTX track. This is referred to as a mis-association. Such mis-associations result in further smearing of the reconstructed and . The FVTX-MuTr association efficiency depends on the event multiplicity. The probability of mis-association can be evaluated with a data driven method developed in [40, 41] by associating a MuTr track with FVTX tracks from another event of similar FVTX track multiplicity. The same method has been used in this analysis, and the estimated fraction of mis-associations in the + data is at \mbox{p_{T}}\approx 1.5~{}{\rm GeV}/c and decreases down to at \mbox{p_{T}}\approx 5~{}{\rm GeV}/c. In the 0%–5% highest multiplicity p$$+Au collisions, the estimated fraction of mis-associations in the south arm (Au-going direction) is at \mbox{p_{T}}\approx 1.5~{}{\rm GeV}/c and at \mbox{p_{T}}\approx 5~{}{\rm GeV}/c, which is a factor of two higher than the estimate for + collisions. The mis-association fraction is also checked with hadron simulation events embedded into real data events, and is consistent with the data driven values. The embedding simulation described in Sec. III.4 is used to take into account the multiplicity dependent FVTX-MuTr association efficiency.
In addition to the requirements on and FVTX-MuTr association, track quality cuts are applied. MuTr tracks are required to have at least 11 hits out of a maximum of 16 hits, and a 3 MuTr track fit quality cut is applied. For association between MuTr and MuID tracks, three standard deviation cuts are applied to the angle and distance between MuTr and MuID tracks projected to the MuID gap 0. The associated FVTX track is required to have hits in at least three of the four stations, and an additional 3 fit quality cut is applied. Momentum-dependent cuts are applied to the angle difference in the radial and azimuthal directions between FVTX and MuTr tracks projected to the middle of the absorber ( cm). These selections help reject tracks from decay muons, secondary hadrons, and FVTX-MuTr mis-associations.
The trigger efficiency is evaluated using hadron candidates from MB triggered events by measuring the fraction of hadron candidates satisfying the trigger requirements. Figure 4 shows the trigger efficiency for hadrons as a function of at MuID gap 2 and gap 3 of the south arm in the + data. The trigger efficiency for hadrons at MuID gap 3 is higher than that for hadrons at MuID gap 2. The efficiency at the north arm in the + data is similar. Due to the larger statistical fluctuations at \mbox{p_{T}}>5~{}{\rm GeV}/c, a fit function is used to obtain the -dependent trigger efficiency correction factors. The trigger efficiency is separately evaluated for each muon arm as well as each centrality bin of p$$+Al and p$$+Au collisions to account for possible multiplicity effects and detector performance variation during the data taking period. The relative variation of the trigger efficiency over the data taking period is less than 10%. Because this variation of the trigger efficiency is accounted for by the detector performance variation described in Sec. III.4, no additional systematic uncertainty is assigned.
III.4 Acceptance and reconstruction efficiency
Calculation of the absolute acceptance and efficiency for hadrons requires a detailed simulation of the hadronic interactions in the thick absorber material. There are significant uncertainties as observed from various geant4 implementations of such interactions. However, the response of hadrons inside the absorber is independent of collision systems, and hence this uncertainty will cancel out when comparing hadron yields between two collision systems. Therefore, nuclear effects on hadron production can be studied by taking into account only the additional multiplicity-dependent efficiency corrections. To obtain the multiplicity-dependent efficiency corrections, a full geant4 detector simulation was developed as follows:
Generate a mixture of hadrons (, , , , , and ) based on initial and distributions studied in [42, 12]. Based on measurements of identified charged hadrons at midrapidity [43, 44, 11], an extrapolation to forward and backward rapidity is done by multiplying the ratio of spectra between mid and forward/backward rapidity from event generators [45, 46]. These simulated hadrons originate from a distribution which matches the measured data. 2. 2.
Run a full geant4 simulation for the detector response of hadrons. 3. 3.
Reconstruct simulated detector hits embedded on top of background hits from real data for each centrality bin in each collision system. Apply the data-driven detector dead channel maps to account for variations in detector performance.
Figure 5 shows an example of acceptance and efficiency result as a function of for different species of hadrons at MuID gaps 2 and 3 of the south arm in + collisions. The acceptance and efficiency for and is comparable, and has the highest acceptance and efficiency due to its longer nuclear interaction length. The acceptance and efficiency for and is much smaller than other charged hadrons.
Due to these species-dependent corrections, the overall acceptance and efficiency will depend on the relative production of these hadrons. In order to correctly account for the species dependence, an initial ratio for each collision system is estimated separately. The contribution of and to reconstructed tracks based on this hadron simulation is less than 5%, and thus we do not include them in the overall result. Figure 6 shows the combined acceptance and efficiency for and as a function of in + collisions for various ranges. The acceptance and efficiency is higher at more forward rapidity where path length through the absorber is shorter, and the total momentum of tracks for a given range is also larger. To have a more accurate correction, the full and dependent correction is applied.
III.5 Nuclear modification factor
Nuclear effects on charged hadron production in p$$+Al and p$$+Au collisions are quantified with the nuclear modification factor,
[TABLE]
where is the charged hadron yield in a certain centrality bin of p$$+Al and p$$+Au collisions. These yields are corrected for the trigger efficiency, acceptance and reconstruction efficiency, and centrality bias factor introduced in Sec. II. is the hadron yield in + collisions corrected for the trigger efficiency, acceptance and reconstruction efficiency, and BBC efficiency. Finally is the mean number of binary collisions for the corresponding centrality bin as calculated with the MC Glauber framework [47]. The values, bias correction factors, and related systematic uncertainties for each centrality bin of p$$+Al and p$$+Au collisions appear in Table 1.
IV Systematic uncertainties
In this section, sources of systematic uncertainty in the nuclear modification factor are described, and the procedure used to determine each systematic uncertainty is discussed.
IV.1 Acceptance and efficiency
IV.1.1 Initial hadron distribution
Because there are limited measurements of identified charged hadrons at forward and backward rapidity (), some model assumptions are necessary. Such forward rapidity particle yields have previously been estimated for use in earlier PHENIX + and d$$+Au collisions studies—see Ref. [12] for details. Here we follow that previous work as input for our simulation studies. To account for uncertainties on the estimated and distributions, weight factors in and for each collision system are extracted by comparing reconstructed and distributions between data and simulation. The variation of acceptance and efficiency with modified initial and distributions based on the weighting factors is less than 3% for + data. For p$$+Al and p$$+Au data, the variation at forward (backward) rapidity is less than 3% (5%). The variation is included in the systematic uncertainty.
In addition, there is an uncertainty in the ratio which influences the combined acceptance and efficiency due to the longer nuclear interaction length of . Based on the uncertainties of measurements at midrapidity [43, 44, 11] used as an input for extrapolation to forward and backward rapidity and a possible extrapolation uncertainty estimated by comparing with the data at more forward rapidity [48], an effect of a 30% variation of on the acceptance and efficiency has been evaluated.
The at midrapidity in various centrality bins of d$$+Au collisions are compatible with each other [11], and the difference of between d$$+Au and p$$+Al and p$$+Au collisions in hijing [46] is less than 10%. These additional sources of uncertainty are covered by the 30% variation of . The variation of acceptance and efficiency due to the 30% change is less than 5% (7%) in + (p$$+Al and p$$+Au) collisions.
IV.1.2 Proton contamination
As described in Sec. III.4, the acceptance and efficiency is calculated for and . There is an proton contamination where the fraction may vary with the initial ratio. Based on the results in + and d$$+Au collisions at midrapidity [43, 44, 11], the ratio at \mbox{p_{T}}\approx 2~{}{\rm GeV}/c in 0%–20% central d$$+Au collisions is about 30% larger than in + collisions, which results in an increase of the contamination to 6.5% in 0%–20% central d$$+Au collisions as compared with 5% in + collisions. However, there is a lack of measurements in a broader range in various centrality ranges of p$$+Al and p$$+Au collisions. Therefore, a conservative uncertainty of 5% is assigned corresponding to a factor of two difference in ratios between p$$+Al, p$$+Au, and + collisions.
IV.1.3 Hadron simulation
Although hadron response inside the absorber will not vary between different collision systems, the variation of acceptance and efficiency among three hadron interaction models (qgsp bert, qgsp bic, and ftfp bert) in geant4 has been checked. A detailed description of the three models and a previous study for muons can be found in Refs. [49, 50]. The variation of the combined acceptance and efficiency for and between the three models is less than 2% in and .
IV.1.4 Variation of detector efficiency
During the data taking period, the detector performance varied due to temporary dead channels, changes in the instantaneous beam luminosity, and other experimental factors. The average detector efficiency for each collision system is included in the hadron simulation. The raw yield variation in FVTX and muon tracks is considered as a source of systematic uncertainty. The level of variation appears in Table 2. The FVTX performance is quite stable during the entire data taking period, and the variation of the muon arm is observed to be larger in the south arm in the p$$+Au data due to a larger sensitivity of the MuID efficiency to the instantaneous beam luminosity of Au ions. A 1 variation of the raw yield is assigned as a systematic uncertainty for each detector, and two systematic uncertainties are added in quadrature.
IV.1.5 FVTX-MuTr mis-association
The probability of FVTX-MuTr mis-association depends on the FVTX track multiplicity, and the mis-association may artificially increase the acceptance and efficiency when requiring FVTX track association. The procedure for calculating the acceptance and efficiency using embedded simulations takes into account the multiplicity dependent FVTX-MuTr mis-association. The primary method to estimate the fraction of FVTX-MuTr is the data driven method described in Sec. III.2, and the systematic uncertainty is evaluated by comparing with the estimated fraction from the embedded simulation. The difference is less than 1% of the maximum of FVTX-MuTr mis-association contamination in 0%–5% p$$+Au collisions. A 1% systematic uncertainty is assigned for the estimation of FVTX-MuTr mis-association.
IV.1.6 Vertex resolution
Because the location of the FVTX is close to the interaction point, the acceptance of the FVTX depends on the position of collisions. In the hadron simulation for acceptance and efficiency calculation, the measured distribution for each collision system is used, but there is uncertainty due to the resolution of . When considering the 2 cm of resolution, the variation of acceptance and efficiency is less than 0.5% in all three collision systems. A 0.5% systematic uncertainty is assigned due to the resolution.
IV.2 Contamination from secondary hadrons
Remaining secondary hadrons can introduce a smearing of kinematic variables ( and ) used in this analysis. The hadron simulation for calculating acceptance and efficiency already includes this component, however there can be a discrepancy in the relative contribution of secondary hadrons between the data and simulation. The systematic uncertainty on is estimated by varying the FVTX-MuTr matching quality cuts (projection angles between FVTX and MuTr tracks) which affect the remaining fraction of secondary hadrons. Based on the hadron simulation, a tighter or looser FVTX-MuTr matching quality cut changes the relative fraction of secondary hadrons by ; the variation on is less than 3%.
IV.3 Multiple collisions
Due to the high instantaneous beam luminosity particularly in + and p$$+Al collisions, there is a chance of having multiple collisions in a single bunch crossing. This can introduce a bias in the yield calculation as well as centrality determination. The effect has been checked by analyzing two data groups with low and high instantaneous beam luminosity, and the difference in is less than 5%. The variation due to multiple collisions is already considered in the systematic uncertainty from the variations in detector efficiency with data-taking period. Therefore, no additional systematic uncertainty is assigned.
IV.4 BBC efficiency and centrality selection
The BBC efficiency in + collisions is for MB events and for hard scattering events, and a 10% systematic uncertainty is assigned based on previous studies [38]. This uncertainty is a global scale uncertainty.
As described in Table 1, there are systematic uncertainties on and bias correction factor calculations. The procedure to estimate these systematic uncertainties has been studied for d$$+Au collisions [39], and the same procedure is used for p$$+Al and p$$+Au collisions.
IV.5 Summary of systematic uncertainty
Table 3 shows the summary of systematic uncertainties. All systematic uncertainties are point-to-point correlated. Because most of sources on the acceptance and efficiency are independent in each collision system, there is no cancellation of systematic uncertainty for calculation.
V Results and Discussion
Figures 7 and 8 show of charged hadrons as a function of at forward and backward rapidity in p$$+Al and p$$+Au collisions at GeV. Both results in 0%–100% centrality are obtained by integrating over all centrality and applying the bias correction factors. Bars (boxes) around the data points represent statistical (systematic) uncertainties, and boxes around unity represent the global systematic uncertainty due to uncertainties in the BBC efficiency and the calculated . The results for p$$+Al indicate that there is little modification at forward rapidity (i.e. in the -going direction), whereas a small enhancement is observed in \mbox{p_{T}}<2~{}{\rm GeV}/c at backward rapidity (i.e. in the Al-going direction). In p$$+Au results, a suppression is seen in \mbox{p_{T}}<3~{}{\rm GeV}/c at forward rapidity unlike the p$$+Al results. At backward rapidity, a similar trend of enhancement is observed in the p$$+Au data, though with larger magnitude.
Comparisons with estimated based on nuclear modified PDFs are shown from the ncteq15 nPDF [22] and the epps16 nPDF [23] interfaced with pythia v8.235 [51]; the parameters used in the event generation of pythia are listed in Table 4. Note that the multiplication factor for multiparton interactions is determined by comparing the -dependent multiplicity distribution in + collisions at GeV [52]. The calculations indicate a modest expected suppression at forward rapidity from shadowing of low- partons in the Au nucleus, and are in agreement with the data within uncertainties. However, at backward rapidity, sensitive to potential anti-shadowing of higher- partons in the Au nucleus, the calculations result in no modification in contradistinction from the data. pQCD calculations considering incoherent multiple scatterings inside the nucleus before and after hard scattering [14] at backward rapidity are also compared with the data, and it agrees with the both p$$+Al and p$$+Au data.
Figure 9 shows of charged hadrons integrated over the interval 2.5<\mbox{p_{T}}<5~{}{\rm GeV}/c as a function of in the 0%–100% centrality selection of (a) p$$+Al and (b) p$$+Au collisions at GeV. Again the data are compared with pQCD calculations at backward rapidity and calculations based on two nPDF sets. In p$$+Au collisions, there is a modest hint that enhancement at backward rapidity becomes larger as approaches midrapidity, while the suppression at forward rapidity becomes stronger. In p$$+Al collisions, at forward rapidity is quite similar to what is observed in p$$+Au collisions, whereas it shows a smaller enhancement at backward rapidity than the results in p$$+Au collisions. The comparison with ncteq15 and epps16 nPDF calculations indicates that the at forward rapidity agrees in both p$$+Al and p$$+Au collisions, but the enhancement at backward rapidity in p$$+Au collisions is not reproduced by the both calculations. In case of the comparison with the pQCD calculations at backward rapidity, the magnitude of enhancement is similar. However, the pQCD calculations show a stronger enhancement at more backward rapidity which is different from the trend in the data.
Because initial and final-state nuclear effects on hadron production may depend on the density of initial partons in the nucleus and on the density of final-state produced particles, has been measured in various centrality bins of p$$+Al and p$$+Au collisions. Figures 11 and 11 show of charged hadrons as a function of or at forward and backward rapidity from the most central bin (0%–5%) to the most peripheral bin (40%–72%) for p$$+Al collisions at GeV. The results at forward and backward rapidity are plotted together in each plot. First, there is a clear centrality dependence both at forward and backward rapidity. The magnitude of the modification, which shows enhancement at backward rapidity and suppression at forward rapidity, becomes stronger in more central p$$+Al collisions. The observed in the most peripheral (40%–72%) p$$+Al collisions is consistent with unity in both rapidity regions, indicating little modification of charged hadron production compared to the + data. Both the magnitude of the modification and the dependence are larger in central collisions. at forward and backward rapidity in central p$$+Au collisions. The centrality dependence of as a function of shown in Fig. 11 is consistent with what is seen in as a function of . The dependence at backward rapidity is weakly centrality dependent, but there is a clear dependence at forward rapidity in the most central collisions.
Figures 13 and 13 show of charged hadrons as a function of and in various centrality classes of p$$+Au collisions. Similar to the results in p$$+Al collisions, the magnitude of modification becomes larger in more central collisions both at forward and backward rapidity, and the values in the most peripheral p$$+Au collisions are consistent with unity. When comparing p$$+Al and p$$+Au results in the 0%–5% central collisions shown in the panel (a) of Figs. 11, 11, 13, and 13, at forward rapidity is comparable between the two collision systems. However, the enhancement at backward rapidity is much stronger in p$$+Au collisions. Figure 13 compares pQCD calculations with the p$$+Au data at backward rapidity. Similarly with the comparison in the integrated centrality, the calculation can reproduce the and centrality dependent enhancement.
Figure 14 shows as a function of for charged hadrons in the range 2.5<\mbox{p_{T}}<5~{}{\rm GeV}/c at (a) forward and (b) backward rapidity in p$$+Al and p$$+Au collisions at GeV. Unlike the previous results, the systematic uncertainty on is included in boxes around data points. The data show that at backward rapidity (filled [black] circles), i.e. in the -going direction, increases monotonically with , and the trend is reproduced by the pQCD calculation. However, at forward rapidity (open [red] circles), i.e. in the -going direction, reveal that each collision system has its own decreasing trend as becomes larger. at forward rapidity in 0%–5% of p$$+Al and p$$+Au collisions are consistent (\mbox{R_{pA}}\sim 0.7), although (9.7 in p$$+Au and 4.1 in p$$+Al collisions) are quite different. The trend of a larger enhancement (suppression) at backward (forward) rapidity in more central collisions is consistent with the previous results of charged hadrons and muons from heavy flavor decay in d$$+Au collisions [31, 12]. A closer look on -dependent in 0%–5% p$$+Al and 40%–60% p$$+Au collisions of similar is shown in Fig. 15. At backward rapidity, it shows not only a consistent magnitude of but also a quite similar trend of in . In case of the comparison at forward rapidity, of the 40%–60% p$$+Au centrality bin is consistent with unity in all bins, whereas a -dependent suppression is seen in 0%–5% p$$+Al collisions.
The suppression of charged hadron production at forward rapidity in integrated centrality of p$$+Al and p$$+Au collisions can be explained by the nPDF modification based on the comparison with the ncteq15 and epps16 calculations shown in Figs 7, 8, and 9. It would be useful to extend another calculation within the CGC framework [27], which successfully describes the suppression of charged hadron production at forward rapidity in d$$+Au collisions [8, 9]. More differential calculations from these various frameworks are needed to compare to the systematic trends found in our new results. In addition to these models which consider modification of the parton distribution functions inside the nucleus, the pQCD calculation of dynamic shadowing considering coherent multiple scatterings inside the nucleus [19] also predicts a rapidity and impact parameter dependent suppression of hadron production at forward rapidity. The centrality dependent suppression at forward rapidity shown in both p$$+Al and p$$+Au collisions also can be described by the color fluctuation effects expecting a stronger centrality dependence in p$$+Au collisions than d$$+Au collisions [30]. It will be quite useful to have theoretical calculations for detailed comparison with the data in , rapidity, and centrality.
For the enhancement of charged hadron production observed at backward rapidity, estimates from the nPDF sets clearly fail to describe the data. A pQCD calculation considering incoherent multiple scatterings both before and after hard scattering [14], which can describe the enhancement of heavy quark production at backward rapidity in d$$+Au collisions [12], successfully explains the centrality and -dependent enhancement. In addition, there is also a possibility of hydrodynamic behavior showing a larger elliptic flow of charged particles at backward rapidity where the multiplicity is also larger than other rapidity ranges [53].
VI Summary
PHENIX has measured the nuclear modification factor of charged hadrons as a function of and at forward and backward rapidity in various centrality ranges of p$$+Al and p$$+Au collisions at GeV. The results in central p$$+Al and p$$+Au collisions show a suppression (enhancement) in the forward -going (backward, -going) rapidity region compared to the binary scaled + results of 0.7 (2.0) for p$$+Au and 0.9 (1.2) for p$$+Al in 2.5<\mbox{p_{T}}<5~{}{\rm GeV}/c at a level of significance () for p$$+Au and () for p$$+Al. In contrast, there is no significant modification of charged hadron production observed in peripheral p$$+Al and p$$+Au collisions in either rapidity region. The enhancement at backward rapidity shows a clear -dependence, but the suppression at forward rapidity is comparable between the two collision systems despite more than a factor two larger in p$$+Au collisions. The results integrated over centrality are compared to a calculation with the ncteq15 and epps16 nPDF sets. The calculation agrees with the data at forward rapidity both in the integrated centrality of p$$+Al and p$$+Au collisions, but it fails to describe the enhancement observed at backward rapidity in p$$+Au collisions. Because the nPDF sets does not yet provide an impact parameter dependent nPDF, the comparison is limited to the case of integrated centrality. These data measured in various centrality ranges can be useful to test impact parameter dependent nPDFs in different nuclei in the future. The pQCD calculation considering incoherent multiple scatterings inside the nucleus can describe the data at backward rapidity. In addition, a comparison with different models can help to improve the understanding of nuclear effects in small collision systems.
Acknowledgements.
We thank the staff of the Collider-Accelerator and Physics Departments at Brookhaven National Laboratory and the staff of the other PHENIX participating institutions for their vital contributions. We thank Z.-B. Kang and H. Xing for useful discussions and for providing theoretical calculations. We acknowledge support from the Office of Nuclear Physics in the Office of Science of the Department of Energy, the National Science Foundation, Abilene Christian University Research Council, Research Foundation of SUNY, and Dean of the College of Arts and Sciences, Vanderbilt University (U.S.A), Ministry of Education, Culture, Sports, Science, and Technology and the Japan Society for the Promotion of Science (Japan), Conselho Nacional de Desenvolvimento Científico e Tecnológico and Fundação de Amparo à Pesquisa do Estado de São Paulo (Brazil), Natural Science Foundation of China (People’s Republic of China), Croatian Science Foundation and Ministry of Science and Education (Croatia), Ministry of Education, Youth and Sports (Czech Republic), Centre National de la Recherche Scientifique, Commissariat à l’Énergie Atomique, and Institut National de Physique Nucléaire et de Physique des Particules (France), Bundesministerium für Bildung und Forschung, Deutscher Akademischer Austausch Dienst, and Alexander von Humboldt Stiftung (Germany), J. Bolyai Research Scholarship, EFOP, the New National Excellence Program (ÚNKP), NKFIH, and OTKA (Hungary), Department of Atomic Energy and Department of Science and Technology (India), Israel Science Foundation (Israel), Basic Science Research and SRC(CENuM) Programs through NRF funded by the Ministry of Education and the Ministry of Science and ICT (Korea). Physics Department, Lahore University of Management Sciences (Pakistan), Ministry of Education and Science, Russian Academy of Sciences, Federal Agency of Atomic Energy (Russia), VR and Wallenberg Foundation (Sweden), the U.S. Civilian Research and Development Foundation for the Independent States of the Former Soviet Union, the Hungarian American Enterprise Scholarship Fund, the US-Hungarian Fulbright Foundation, and the US-Israel Binational Science Foundation.
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