STAR Collaboration

Adamczyk, L.; Adkins, J.K.; Agakishiev, G.; Aggarwal, M.M.; Ahammed, Z.; Alekseev, I.; Aparin, A.; Arkhipkin, D.; Aschenauer, E.C.; Ashraf, M.U.; Attri, A.; Averichev, G.S.; Bai, X.; Bairathi, V.; Bellwied, R.; Bhasin, A.; Bhati, A.K.; P., Bhattarai,; Bielcik, J.; Bielcikova, J.; Bland, L.C.; Bordyuzhin, I.G.; Bouchet, J.; Brandenburg, J.D.; Brandin, A.V.; Bunzarov, I.; Butterworth, J.; Caines, H.; Sánchez, M. Calderón De La Barca; Campbell, J.M.; Cebra, D.; Chakaberia, I.; Chaloupka, P.; Chang, Z.; Chatterjee, A.; Chattopadhyay, S.; Chen, X.; Chen, J.H.; Cheng, J.; Cherney, M.; Christie, W.; Contin, G.; Crawford, H.J.; Das, S.; Silva, L.C. De; Debbe, R.R.; Dedovich, T.G.; Deng, J.; Derevschikov, A.A.; Ruzza, B. Di; Didenko, L.; Dilks, C.; Dong, X.; Drachenberg, J.L.; Draper, J.E.; Du, C.M.; Dunkelberger, L.E.; Dunlop, J.C.; Efimov, L.G.; Engelage, J.; Eppley, G.; Esha, R.; Evdokimov, O.; Eyser, O.; Fatemi, R.; Fazio, S.; Federic, P.; Fedorisin, J.; Feng, Z.; Filip, P.; Fisyak, Y.; Flores, C.E.; Fulek, Ł.; Gagliardi, C.A.; Garand, D.; F., Geurts,; Gibson, A.; Girard, M.; Greiner, L.; Grosnick, D.; Gunarathne, D.S.; Guo, Y.; Gupta, S.; Gupta, A.; Guryn, W.; Hamad, A.I.; Hamed, A.; Haque, R.; Harris, J.W.; He, L.; Heppelmann, S.; Hirsch, A.; Hoffmann, G.W.; Horvat, S.; Huang, T.; Huang, B.; Huang, X.; Huang, H.Z.; Huck, P.; Humanic, T.J.; Igo, G.; Jacobs, W.W.; Jang, H.; Jentsch, A.; Jia, J.; Jiang, K.; Judd, E.G.; Kabana, S.; Kalinkin, D.; Kang, K.; Kauder, K.; Ke, H.W.; Keane, D.; Kechechyan, A.; Khan, Z.H.; Kikoła, D. P.; Kisel, I.; Kisiel, A.; Kochenda, L.; Koetke, D.D.; Kosarzewski, L.K.; Kraishan, A.F.; Kravtsov, P.; Krueger, K.; Kumar, L.; Lamont, M.A.C.; Landgraf, J.M.; Landry, K.D.; Lauret, J.; Lebedev, A.; Lednicky, R.; Lee, J.H.; Li, X.; Li, Y.; Li, C.; Li, W.; Li, X.; Lin, T.; Lisa, M.A.; Liu, F.; Ljubicic, T.; Llope, W.J.; Lomnitz, M.; Longacre, R.S.; Luo, X.; Luo, S.; Ma, G.L.; Ma, L.; Ma, Y.G.; Ma, R.; Magdy, N.; Majka, R.; Manion, A.; Margetis, S.; Markert, C.; Matis, H.S.; McDonald, D.; McKinzie, S.; Meehan, K.; Mei, J.C.; Miller, Z.W.; Minaev, N.G.; Mioduszewski, S.; Mishra, D.; Mohanty, B.; Mondal, M.M.; Morozov, D.A.; Mustafa, M.K.; Nandi, B.K.; Nasim, Md.; Nayak, T.K.; Nigmatkulov, G.; Niida, T.; Nogach, L.V.; Noh, S.Y.; Novak, J.; Nurushev, S.B.; Odyniec, G.; Ogawa, A.; Oh, K.; Okorokov, V.A.; Olvitt, D.; Page, B.S.; Pak, R.; Pan, Y.X.; Pandit, Y.; Panebratsev, Y.; Pawlik, B.; Pei, H.; Perkins, C.; Pile, P.; Pluta, J.; Poniatowska, K.; Porter, J.; Posik, M.; Poskanzer, A.M.; Pruthi, N.K.; Przybycien, M.; Putschke, J.; Qiu, H.; Quintero, A.; Ramachandran, S.; Ray, R.L.; Reed, R.; Ritter, H.G.; Roberts, J.B.; Rogachevskiy, O.V.; Romero, J.L.; Ruan, L.; Rusnak, J.; Rusnakova, O.; Sahoo, N.R.; Sahu, P.K.; Sakrejda, I.; Salur, S.; Sandweiss, J.; Sarkar, A.; Schambach, J.; Scharenberg, R.P.; Schmah, A.M.; Schmidke, W.B.; Schmitz, N.; Seger, J.; Seyboth, P.; Shah, N.; Shahaliev, E.; Shanmuganathan, P.V.; Shao, M.; Sharma, A.; Sharma, B.; Sharma, M.K.; Shen, W.Q.; Shi, Z.; Shi, S.S.; Shou, Q.Y.; Sichtermann, E.P.; Sikora, R.; Simko, M.; Singha, S.; Skoby, M.J.; Smirnov, D.; Smirnov, N.; Solyst, W.; Song, L.; Sorensen, P.; Spinka, H.M.; Srivastava, B.; Stanislaus, T.D.S.; Stepanov, M.; Stock, R.; Strikhanov, M.; Stringfellow, B.; Šumbera, M.; Summa, B.; Sun, Y.; Sun, Z.; Sun, X.M.; Surrow, B.; Svirida, D. N.; Tang, Z.; Tang, A.H.; Tarnowsky, T.; Tawfik, A.; Thäder, J.; Thomas, J.H.; Timmins, A.R.; Tlusty, D.; Todoroki, T.; Tokarev, M.; Trentalange, S.; Tribble, R.E.; Tribedy, P.; Tripathy, S.K.; Tsai, O.D.; Ullrich, T.; Underwood, D.G.; Upsal, I.; Buren, G. Van; Nieuwenhuizen, G. van; Vandenbroucke, M.; Varma, R.; Vasiliev, A.N.; Vertesi, R.; Videbæk, F.; Vokal, S.; Voloshin, S.A.; Vossen, A.; Wang, H.; Wang, F.; Wang, Y.; Wang, J.S.; Wang, G.; Wang, Y.; Webb, J.C.; Webb, G.; Wen, L.; Westfall, G.D.; Wieman, H.; Wissink, S.W.; Witt, R.; Wu, Y.; Xiao, Z.G.; Xie, W.; Xie, G.; Xin, K.; Xu, N.; Xu, Q.H.; Xu, Z.; Xu, J.; Xu, H.; Xu, Y.F.; Yang, S.; Yang, C.; Yang, Y.; Yang, Q.; Ye, Z.; Ye, Z.; Yi, L.; Yip, K.; Yoo, I.-K.; Yu, N.; Zbroszczyk, H.; Zha, W.; Zhang, Z.; Zhang, J.B.; Zhang, S.; Zhang, S.; Zhang, X.P.; Zhang, Y.; Zhang, J.; Zhang, J.; Zhao, J.; Zhong, C.; Zhou, L.; Zhu, X.; Zoulkarneeva, Y.; Zyzak, M.

doi:10.1016/s0375-9474(17)30384-6

Cited by 287 publications

(699 citation statements)

References 0 publications

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“…For the antiproton slopes we again observe an almost quantitative agreement with the BES experiment (Adamczyk et al 2014): With increasing collision energy, the HSD and PHSD slopes grow and then flatten above 20-30 GeV. The HSD results saturate at v 1 (0) = 0, while the PHSD predictions stay negative and in good agreement with experiment (see Fig.…”

Section: Directed Flowsupporting

confidence: 82%

“…However, the absolute values of the calculated proton slopes in this high energy range are on the level of -(0.010-0.015), while the measured ones are about -0.005. The standard UrQMD model results, as cited in the experimental paper (Adamczyk et al 2014) and in the more recent theoretical work (Steinheimer et al 2014), are displayed in Fig. 3 by the wide and narrow shaded areas, respectively.…”

Section: Directed Flowmentioning

confidence: 91%

“…The average impact parameter for the selected events is b = 7 fm. In the simulations the experimental acceptance 0.2 ≥ p T ≥ 2 GeV/c is taken into account for all hadrons (Adamczyk et al 2014). Note that the PHSD/HSD calculations in Figs.…”

Section: Directed Flowmentioning

confidence: 99%

“…Note that the energy axis in Fig. 3 is extended by adding experimental results for √ s NN = 62 and 200 GeV (Adamczyk et al 2014). This representation is more delicate as compared to v 1 (y) in Fig.…”

Section: Directed Flowmentioning

confidence: 99%

“…The interest in the directed flow v 1 (y) has been enhanced considerably due to new STAR data obtained in the framework of the beam energy scan (BES) program (Adamczyk et al 2014). The directed flow of identified hadrons -protons, antiprotons, positive and negative pions -has been measured with high precision for semi-central Au+Au collisions in the energy range √ s NN = 7.7-39 GeV.…”

Section: Introductionmentioning

confidence: 99%

See 4 more Smart Citations

From cold to hot nuclear matter

et al. 2015

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The dynamics of partons and hadrons in relativistic nucleus-nucleus collisions is analyzed within the Parton-Hadron-String Dynamics (PHSD) transport approach which is based on a dynamical quasiparticle model for the partonic phase (DQPM) including a dynamical hadronization scheme with covariant transition rates. The PHSD approach is applied to nucleus-nucleus collisions from FAIR/NICA to LHC energies. The traces of partonic interactions are found in particular in the directed and elliptic flow of hadrons and in their transverse mass spectra. Whereas at RHIC and LHC energies the dynamics is dominated by partonic degrees-of-freedom in the hot QGP, we find at FAIR/NICA energies a moderately hot but dense matter where chiral symmetry restoration and hadronic potentials appear to play a major role.

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Section: Directed Flowsupporting

confidence: 82%

Section: Directed Flowmentioning

confidence: 91%

Section: Directed Flowmentioning

confidence: 99%

Section: Directed Flowmentioning

confidence: 99%

Section: Introductionmentioning

confidence: 99%

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From cold to hot nuclear matter

et al. 2015

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Degrees of Freedom of the Quark Gluon Plasma, Tested by Heavy Mesons

Berrehrah

Nahrgang

Song

et al. 2016

New Horizons in Fundamental Physics

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Heavy quarks (charm and bottoms) are one of the few probes which are sensitive to the degrees of freedom of a Quark Gluon Plasma (QGP), which cannot be revealed by lattice gauge calculations in equilibrium. Due to the rapid expansion of the QGP energetic heavy quarks do not come to an equilibrium with the QGP. Their energy loss during the propagation through the QGP medium depends strongly on the modelling of the interaction of the heavy quarks with the QGP quarks and gluons, i.e. on the assuption of the degrees of freedom of the plasma. Here we compare the results of different models, the pQCD based Monte-Carlo (MC@sHQ), the Dynamical Quasi Particle Model (DQPM) and the effective mass approach, for the

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Anomalous effects of dense matter under rotation

Huang

Nishimura

Yamamoto

2018

J. High Energ. Phys.

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We study the anomaly induced effects of dense baryonic matter under rotation. We derive the anomalous terms that account for the chiral vortical effect in the low-energy effective theory for light Nambu-Goldstone modes. The anomalous terms lead to new physical consequences, such as the anomalous Hall energy current and spontaneous generation of angular momentum in a magnetic field (or spontaneous magnetization by rotation). In particular, we show that, due to the presence of such anomalous terms, the ground state of the quantum chromodynamics (QCD) under sufficiently fast rotation becomes the "chiral soliton lattice" of neutral pions that has lower energy than the QCD vacuum and nuclear matter. We briefly discuss the possible realization of the chiral soliton lattice induced by a fast rotation in noncentral heavy ion collisions.

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STAR Collaboration

Cited by 287 publications

References 0 publications

From cold to hot nuclear matter

From cold to hot nuclear matter

Degrees of Freedom of the Quark Gluon Plasma, Tested by Heavy Mesons

Anomalous effects of dense matter under rotation

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