PHENIX Collaboration

Adare, A.; Afanasiev, S.; C., Aidala,; Ajitanand, N.N.; Akiba, Y.; Akimoto, R.; Al-Bataineh, H.; Alexander, J.; Alfred, M.; Al-Jamel, A.; Al-Ta'ani, H.; Andrews, K.R.; Andrieux, V.; Angerami, A.; Aoki, K.; Apadula, N.; Aphecetche, L.; Appelt, E.; Aramaki, Y.; Armendariz, R.; Aronson, S.H.; Asai, J.; Asano, H.; Aschenauer, E.C.; Atomssa, E.T.; Averbeck, R.; Awes, T.C.; Azmoun, B.; Babintsev, V.; Bai, M.; Bai, X.; Baksay, G.; Baksay, L.; Baldisseri, A.; Bandara, N.S.; Bannier, B.; Barish, K.N.; Barnes, P.D.; Bassalleck, B.; Basye, A.T.; Bathe, S.; Batsouli, S.; Baublis, V.; Bauer, F.; Baumann, C.; Baumgart, S.; A., Bazilevsky,; Beaumier, M.; S., Beckman,; Belikov, S.; Belmont, R.; J., Ben-Benjamin,; Bennett, R.; Berdnikov, A.; Berdnikov, Y.; Bhom, J.; Bickley, A.A.; Bjorndal, M.T.; Black, D.; Blau, D.S.; Boissevain, J.G.; Bok, J.S.; Borel, H.; Boyle, K.; Brooks, M.L.; Brown, D.S.; Broxmeyer, D.; Bryslawskyj, J.; Bucher, D.; Buesching, H.; Bumazhnov, V.; Bunce, G.; Burward-Hoy, J.M.; Butsyk, S.; Camacho, C.M.; Campbell, S.; Caringi, A.; Castera, P.; Cervantes, R.; Chai, J.-S.; Chang, B.S.; Chang, W.C.; Charvet, J.-L.; Chen, C.-H.; Chernichenko, S.; Chi, C.Y.; Chiba, J.; Chiu, M.; Choi, I.J.; Choi, J.B.; Choi, S.; Choudhury, R.K.; Christiansen, P.; Chujo, T.; Chung, P.; Churyn, A.; Chvala, O.; V., Cianciolo,; Citron, Z. H.; Cleven, C.R.; Cobigo, Y.; Cole, B.A.; Comets, M.P.; Valle, Z. Conesa del; Connors, M.; Constantin, P.; Cronin, N.; Crossette, N.; Csanád, M.; Csörgő, T.; Dahms, T.; Dairaku, S.; Danchev, I.; Danley, T.W.; Das, K.; A., Datta,; Daugherity, M.S.; David, G.; Dayananda, M.K.; Deaton, M.B.; DeBlasio, K.; Dehmelt, K.; Delagrange, H.; Denisov, A.; d’Enterria, D.; A., Deshpande,; Desmond, E.J.; Dharmawardane, K.V.; Dietzsch, O.; Ding, L.; Dion, A.; Diss, P.B.; Dixit, D.; Dixit, D.D.; Do, J.H.; Donadelli, M.; D'Orazio, L.; Drachenberg, J.L.; Drapier, O.; Drees, A.; Drees, K.A.; Dubey, A.K.; Durham, J.M.; Durum, A.; D., Dutta,; Dzhordzhadze, V.; Edwards, S.; Efremenko, Y.V.; Egdemir, J.; Ellinghaus, F.; Emam, W.S.; Engelmore, T.; Enokizono, A.; H., En'yo,; Espagnon, B.; Esumi, S.; Eyser, K.O.; Fadem, B.; Fan, W.; Feege, N.; Fields, D.E.; Finger, M.; F., Fleuret,; Fokin, S.L.; Forestier, B.; Fraenkel, Z.; Frantz, J.E.; Franz, A.; Frawley, A.D.; Fujiwara, K.; Y., Fukao,; Fukuda, Y.; Fung, S.-Y.; Fusayasu, T.; Gadrat, S.; Gainey, K.; Gal, C.; Gallus, P.; Garg, P.; Garishvili, A.; Garishvili, I.; Gastineau, F.; H., Ge,; Germain, M.; Giordano, F.; Glenn, A.; Gong, H.; Gong, X.; M., Gonin,; Gosset, J.; Goto, Y.; Cassagnac, R. Granier de; Grau, N.; Greene, S.V.; Grim, G.; Perdekamp, M. Grosse; Gu, Y.; T., Gunji,; Guo, L.; Guragain, H.; Gustafsson, H.-Å.; T., Hachiya,; Henni, A. Hadj; Haegemann, C.; Haggerty, J.S.; Hagiwara, M.N.; Hahn, K.I.; Hamagaki, H.; Hamblen, J.; Hamilton, H.F.; Han, R.; Han, S.Y.; Hanks, J.; Harada, H.; Harper, C.; Hartouni, E.P.; Haruna, K.; Harvey, M.; Hasegawa, S.; Haseler, T.O.S.; Hashimoto, K.; Haslum, E.; Hasuko, K.; Hayano, R.; Hayashi, S.; He, X.; Heffner, M.; Hemmick, T.K.; T., Hester,; Heuser, J.M.; Hiejima, H.; Hill, J.C.; Hill, K.; Hobbs, R.; Hohlmann, M.; Hollis, R.S.; Holmes, M.; Holzmann, W.; Homma, K.; Hong, B.; Horaguchi, T.; Hori, Y.; Hornback, D.; Hoshino, T.; Hotvedt, N.; J., Huang,; Huang, S.; Hur, M.G.; Ichihara, T.; Ichimiya, R.; Ide, J.; Iinuma, H.; Ikeda, Y.; Imai, K.; Imazu, Y.; Imrek, J.; Inaba, M.; Inoue, Y.; Iordanova, A.; Isenhower, D.; Isenhower, L.; Ishihara, M.; Isinhue, A.; Isobe, T.; M., Issah,; Isupov, A.; Ivanishchev, D.; Iwanaga, Y.; Jacak, B.V.; Javani, M.; Jeon, S.J.; Jezghani, M.; Jia, J.; Jiang, X.; Jin, J.; Jinnouchi, O.; John, D.; Johnson, B.M.; T., Jones,; Joo, E.; Joo, K.S.; Jouan, D.; Jumper, D.S.; Kajihara, F.; Kametani, S.; Kamihara, N.; Kamin, J.; Kanda, S.; Kaneta, M.; Kaneti, S.; Kang, B.H.; Kang, J.H.; Kang, J.S.; Kanou, H.; Kapukchyan, D.; Kapustinsky, J.; Karatsu, K.; Karthas, E.; M., Kasai,; Kawagishi, T.; Kawall, D.; Kawashima, M.; Kazantsev, A.V.; Kelly, S.; Kempel, T.; Key, J.A.; V., Khachatryan,; Khandai, P. K.; Khanzadeev, A.; Kihara, K.; Kijima, K.M.; Kikuchi, J.; Kim, A.; Kim, B.I.; Kim, C.; Kim, D.H.; Kim, D.J.; Kim, E.; Kim, E.-J.; Kim, G.W.; Kim, H.-J.; Kim, H.J.; Kim, K.-B.; Kim, M.; Kim, S.H.; Kim, Y.-J.; Kim, Y.K.; Kim, Y.-S.; Kimelman, B.; Kincses, D.; Kinney, E.; Kiriluk, K.; Kiss, Á.; E., Kistenev,; R., Kitamura,; Kiyomichi, A.; Klatsky, J.; Klay, J.; Klein-Boesing, C.; Kleinjan, D.; Kline, P.; Koblesky, T.; L., Kochenda,; Kochetkov, V.; Kofarago, M.; Komatsu, Y.; B., Komkov,; Konno, M.; Koster, J.; Kotchetkov, D.; Kotov, D.; Kozlov, A.; Král, A.; Kravitz, A.; Krizek, F.; Kroon, P.J.; Kubart, J.; S., Kudo,; Kunde, G.J.; Kurihara, N.; K., Kurita,; Kurosawa, M.; Kweon, M.J.; Kwon, Y.; Kyle, G.S.; Lacey, R.; Lai, Y.S.; Lajoie, J.G.; Layton, D.; Lebedev, A.; Bornec, Y. Le; Leckey, S.; Lee, B.; Lee, D.M.; Lee, G.H.; Lee, J.; Lee, K.; Lee, K.B.; Lee, K.S.; Lee, M.K.; Lee, S.; Lee, S.H.; Lee, S.R.; Lee, T.; Leitch, M.J.; Leite, M.A.L.; Leitgab, M.; Leitner, E.; Lenzi, B.; Leung, Y.H.; Lewis, B.; Li, X.; Li, X.H.; Lichtenwalner, P.; Liebing, P.; Lim, H.; Lim, S.H.; Levy, L. A. Linden; Liška, T.; Litvinenko, A.; Liu, H.; Liu, M.X.; Loggins, V.-R.; Lovasz, K.; Love, B.; Luechtenborg, R.; Lynch, D.; Maguire, C.F.; Majoros, T.; Makdisi, Y.I.; Makek, M.; Malakhov, A.; Malik, M.D.; Manion, A.; Manko, V.I.; Mannel, E.; Mao, Y.; Maruyama, T.; Mašek, L.; Masui, H.; Masumoto, S.; Matathias, F.; McCain, M.C.; McCumber, M.; McGaughey, P.L.; McGlinchey, D.; McKinney, C.; Means, N.; Meles, A.; Mendoza, M.; Meredith, B.; Miake, Y.; Mibe, T.; Midori, J.; Mignerey, A.C.; Mikeš, P.; Miki, K.; Miller, A.J.; Miller, T.E.; Milov, A.; Mioduszewski, S.; Mishra, D.K.; Mishra, G.C.; Mishra, M.; Mitchell, J.T.; Mitrovski, M.; Mitsuka, G.; Miyachi, Y.; Miyasaka, S.; Mizuno, S.; Mohanty, A.K.; Mohapatra, S.; Montuenga, P.; Moon, H.J.; Moon, T.; Morino, Y.; Morreale, A.; Morrison, D.P.; Moskowitz, M.; Moss, J.M.; Motschwiller, S.; Moukhanova, T.V.; Mukhopadhyay, D.; Murakami, T.; Murata, J.; Mwai, A.; Nagae, T.; Nagai, K.; Nagamiya, S.; Nagashima, K.; Nagashima, T.; Nagata, Y.; Nagle, J.L.; Naglis, M.; Nagy, M.I.; Nakagawa, I.; Nakagomi, H.; Nakamiya, Y.; Nakamura, K.R.; Nakamura, T.; K., Nakano,; Nam, S.; Nattrass, C.; Nederlof, A.; Netrakanti, P.K.; Newby, J.; Nguyen, M.; Nihashi, M.; Niida, T.; Nishimura, S.; Norman, B.E.; Nouicer, R.; Novák, T.; Novitzky, N.; Nukariya, A.; Nyanin, A.S.; Nystrand, J.; Oakley, C.; Obayashi, H.; O'Brien, E.; Oda, S.; Ogilvie, C.A.; Ohnìshì, H.; Oide, H.; Ojha, I.D.; Oka, M.; Okada, K.; Omiwade, O.O.; Onuki, Y.; Koop, J. D. Orjuela; Osborn, J. D.; Oskarsson, A.; Otterlund, I.; Ottino, G.J.; Ouchida, M.; Ozawa, K.; Pak, R.; Pal, D.; Palounek, A.P.T.; Pantuev, V.; Papavassiliou, V.; Park, B.H.; Park, I.H.; Park, J.; Park, J.S.; Park, S.; Park, S.K.; Park, W.J.; Pate, S.F.; L., Patel,; Patel, M.; Pei, H.; Peng, J.-C.; Pereira, H.; Perepelitsa, D.V.; Perera, G.D.N.; Peresedov, V.; Peressounko, D.Yu.; PerezLara, C.E.; Perry, J.; R., Petti,; Phipps, M.; Pinkenburg, C.; R., Pinson,; Pisani, R.P.; Proissl, M.; Purschke, M.L.; Purwar, A.K.; H., Qu,; Rak, J.; Rakotozafindrabe, A.; Ramson, B.J.; Ravinovich, I.; Read, K.F.; Rembeczki, S.; Reuter, M.; Reygers, K.; D., Reynolds,; Riabov, V.; Y., Riabov,; Richardson, E.; Rinn, T.; N., Riveli,; Roach, D.; Roche, G.; Rolnick, S.D.; Romana, A.; Rosati, M.; Rosen, C.A.; Rosendahl, S.S.E.; Rosnet, P.; Z., Rowan,; Rubin, J.G.; Rukoyatkin, P.; Ružička, P.; Rykov, V.L.; Ryu, M.S.; Ryu, S.S.; Safonov, A.S.; Sahlmueller, B.; Saito, N.; Sakaguchi, T.; Sakai, S.; Sakashita, K.; Sakata, H.; Sako, H.; V., Samsonov,; Sano, M.; S., Sano,; M., Sarsour,; Sato, H.D.; S., Sato,; Sato, T.; Savastio, M.; Sawada, S.; B., Schaefer,; Schmoll, B.K.; Sedgwick, K.; Seele, J.; R., Seidl,; Sekiguchi, Y.; Semenov, A.Yu.; Semenov, V.; Sen, A.; Seto, R.; Sett, P.; Sexton, A.; Sharma, D.; Shaver, A.; Shea, T.K.; Shein, I.; Shevel, A.; Shibata, T.-A.; Shigaki, K.; Shim, H.H.; Shimomura, M.; Shioya, T.; Shohjoh, T.; K., Shoji,; Shukla, P.; Sickles, A.; Silva, C.L.; Silvermyr, D.; Silvestre, C.; Sim, K.S.; Singh, B.K.; Singh, C.P.; Singh, V.; Skolnik, M.; Skutnik, S.; Slunečka, M.; Smith, W.C.; Snowball, M.; Sodre, T.; Solano, S.; Soldatov, A.; Soltz, R. A.; Sondheim, W.E.; Sorensen, S.P.; Sourikova, I.V.; Sparks, N.A.; Staley, F.; Stankus, P.W.; Steinberg, P.; Stenlund, E.; Stepanov, M.; Ster, A.; Stoll, S.P.; Stone, M.R.; Sugitate, T.; Suire, C.; Sukhanov, A.; Sullivan, J.P.; T., Sumita,; Sun, J.; Sziklai, J.; Tabaru, T.; Takagi, S.; Takagui, E.M.; Takahara, A.; Taketani, A.; Tanabe, R.; Tanaka, K.H.; Tanaka, Y.; Taneja, S.; Tanida, K.; Tannenbaum, M.J.; Tarafdar, S.; Taranenko, A.; Tarján, P.; Tarnai, G.; Tennant, E.; Themann, H.; Thomas, D.; Thomas, T.L.; Tieulent, R.; Timilsina, A.; Todoroki, T.; Togawa, M.; Toia, A.; Tojo, J.; Tomášek, L.; Tomášek, M.; Tomita, Y.; Torii, H.; Towell, C.L.; Towell, M.; Towell, R.; Towell, R.S.; Tram, V.-N.; Tserruya, I.; Tsuchimoto, Y.; Tsuji, T.; Tuli, S.K.; Tydesjö, H.; Tyurin, N.; Ueda, Y.; B., Ujvari,; Utsunomiya, K.; Vale, C.; Valle, H.; Hecke, H.W. van; Vargyas, M.; Vazquez-Zambrano, E.; Veicht, A.; Velkovska, J.; Vértesi, R.; Vinogradov, A.A.; Virius, M.; Voas, B.; Vossen, A.; Vrba, V.; Vukman, N.; Vznuzdaev, E.; Wagner, M.; Walker, D.; Wang, X.R.; Watanabe, D.; Watanabe, K.; Watanabe, Y.; Watanabe, Y.S.; Wei, F.; Wei, R.; J., Wessels,; Whitaker, S.; White, A.S.; White, S.N.; Willis, N.; Winter, D.; Wolin, S.; Wong, C.P.; Wood, J.P.; Woody, C.L.; Wright, R.M.; Wysocki, M.; Xia, B.; Xie, W.; Xu, C.; Xu, Q.; Xue, L.; Yalcin, S.; Yamaguchi, Y.L.; H., Yamamoto,; Yamaura, K.; Yang, R.; Yanovich, A.; Yasin, Z.; Ying, J.; Yokkaichi, S.; Yoo, J.H.; Yoo, J.S.; Yoon, I.; You, Z.; Young, G.R.; Younus, I.; Yu, H.; Yushmanov, I.E.; Zajc, W.A.; Zaudtke, O.; Zelenski, A.; Zhang, C.; Zhou, S.; Zimamyi, J.; Zolin, L.; Zou, L.

doi:10.1016/s0375-9474(16)30234-2

Cited by 53 publications

(112 citation statements)

References 0 publications

Supporting

Mentioning

105

Contrasting

Order By: Relevance

“…6 one finds that the value of S 0 corresponds to a freeze-out temperature of 153.5(2.0) MeV. This temperature range is consistent with an earlier determination of the freeze-out temperature that was based on a comparison of the mean over variance ratio of net electric-charge and net proton-number ratios obtained by the STAR and PHENIX Collaborations [29,30] with corresponding lattice QCD calculations for net electric-charge and net baryon-number cumulant ratios [31]. We also note that the ratio of the curvature of R B 42 and R B 31 on the pseudo-critical (freeze-out) line tends to be larger than 3, which also has been noted in our previous analysis of skewness and kurtosis ratios [19].…”

Section: Baryon-number Fluctuations On the Pseudo-critical Line Asupporting

confidence: 88%

“…10 thus may be considered only as a starting point for a more refined analysis of the experimental data that may take into account effects arising from experimental acceptance cuts, the small size of the hot and dense medium, non-equilibrium effects etc. 6 Statistics at √ s N N = 54.4 GeV is a factor 3.4 larger than at √ s N N = 200 GeV and a factor (17)(18)(19)(20)(21)(22)(23)(24)(25)(26)(27)(28)(29)(30) larger than at the other √ s N N data sets shown in Fig. 10.…”

Section: Baryon-number Fluctuations On the Pseudo-critical Line Amentioning

confidence: 78%

See 1 more Smart Citation

Skewness, kurtosis, and the fifth and sixth order cumulants of net baryon-number distributions from lattice QCD confront high-statistics STAR data

et al. 2020

View full text Add to dashboard Cite

We present new results on up to 6 th order cumulants of net baryon-number fluctuations at small values of the baryon chemical potential, µB, obtained in lattice QCD calculations with physical values of light and strange quark masses. Representation of the Taylor expansions of higher order cumulants in terms of the ratio of the two lowest order cumulants, MB/σ 2, allows for a parameter free comparison with data on net proton-number cumulants obtained by the STAR Collaboration in the Beam Energy Scan at RHIC. We show that recent high statistics data on skewness and kurtosis ratios of net proton-number distributions, obtained at beam energy √ s N N = 54.4 GeV, agree well with lattice QCD results on cumulants of net baryon-number fluctuations close to the pseudo-critical temperature, Tpc(µB), for the chiral transition in QCD. We also present first results from a next-to-leading order expansion of 5 th and 6 th order cumulants on the line of pseudo-critical temperatures.

show abstract

Section: Baryon-number Fluctuations On the Pseudo-critical Line Asupporting

confidence: 88%

Section: Baryon-number Fluctuations On the Pseudo-critical Line Amentioning

confidence: 78%

Skewness, kurtosis, and the fifth and sixth order cumulants of net baryon-number distributions from lattice QCD confront high-statistics STAR data

et al. 2020

View full text Add to dashboard Cite

show abstract

“…14 In this section we investigate the possible role of nucleon substructure in flow signature of 16 O + 16 O collisions. We compare the predictions of the wounded nucleon model and the wounded parton (wounded quark) model [55][56][57][58] with three constituents, which has turned out successful phenomenologically in explaining the RHIC and LHC data [59][60][61][62][63][64][65][66][67]. The wounded parton picture is implemented in GLISSANDO 3 [18] by placing three partons around the center of each nucleon with an appropriate exponential distribution.…”

Section: Glauber Modelingmentioning

confidence: 99%

Glauber Monte Carlo predictions for ultrarelativistic collisions with O16

Rybczyński

Broniówski

2019

Phys. Rev. C

View full text Add to dashboard Cite

We explore Glauber Monte Carlo predictions for the planned ultra-relativistic 16 O+ 16 O and p+ 16 O collisions, as well as for collisions of 16 O on heavy targets. In particular, we present specific collective flow measures which are approximately independent on the hydrodynamic response of the system, such as the ratios of eccentricities obtained from cumulants with different numbers of particles, or correlations of ellipticity and triangularity described by the normalized symmetric cumulants. We use the state-of-the-art correlated nuclear distributions for 16 O and compare the results to the uncorrelated case, finding moderate effects for the most central collisions. We also consider the wounded quark model, which turns out to yield similar results to the wounded nucleon model for the considered measures. The purpose of our study is to prepare some ground for the upcoming experimental proposals, as well as to provide input for possible more detailed dynamical studies with hydrodynamics or transport codes.

show abstract

“…On the experimental side, heavy ion collisions at various collision energies and several system sizes are carried out in order to probe a wide range in both temperature and baryon chemical potential. Those include the beam energy scan performed at RHIC [7,8,9] and the CERN-SPS [10,11,12]. In the future, this region will be studied further by CBM at FAIR and at NICA.…”

Section: Introductionmentioning

confidence: 99%

Particle production via strings and baryon stopping within a hadronic transport approach

Mohs

Ryu

Elfner

2020

J. Phys. G: Nucl. Part. Phys.

View full text Add to dashboard Cite

The stopping of baryons in heavy ion collisions at beam momenta of p lab = 20 − 160A GeV is lacking a quantitative description within theoretical calculations. Heavy ion reactions at these energies are experimentally explored at the Super Proton Synchrotron (SPS) and the Relativistic Heavy Ion Collider (RHIC) and will be studied at future facilities such as FAIR and NICA. Since the net baryon density is determined by the amount of stopping, this is the pre-requisiste for any investigation of other observables related to structures in the QCD phase diagram such as a first-order phase transition or a critical endpoint. In this work we employ a string model for treating hadron-hadron interactions within a hadronic transport approach (SMASH, Simulating Many Accelerated Strongly-interacting Hadrons). Free parameters of the string excitation and decay are tuned to match experimental measurements in elementary proton-proton collisions. Afterwards, the model is applied to heavy ion collisions, where the experimentally observed change of the shape of the proton rapidity spectrum from a single peak structure to a double peak structure with increasing beam energy is reproduced. Heavy ion collisions provide the opportunity to study the formation process of string fragments in terms of formation times and reduced interaction cross-sections for pre-formed hadrons. A good agreement with the measured rapidity spectra of protons and pions is achieved while insights on the fragmentation process are obtained. In the future, the presented approach can be used to create event-by-event initial conditions for hybrid calculations.

show abstract

PHENIX Collaboration

Cited by 53 publications

References 0 publications

Skewness, kurtosis, and the fifth and sixth order cumulants of net baryon-number distributions from lattice QCD confront high-statistics STAR data

Skewness, kurtosis, and the fifth and sixth order cumulants of net baryon-number distributions from lattice QCD confront high-statistics STAR data

Glauber Monte Carlo predictions for ultrarelativistic collisions with O16

Particle production via strings and baryon stopping within a hadronic transport approach

Contact Info

Product

Resources

About