000030448 001__ 30448
000030448 005__ 20140130020839.0
000030448 037__ $$9arXiv$$aarXiv:1001.5052$$cnucl-ex
000030448 035__ $$9arXiv$$zoai:arXiv.org:1001.5052
000030448 035__ $$9DESY$$zD10-01466
000030448 035__ $$9SPIRESTeX$$zAbelev:2010tr
000030448 100__ $$aAbelev, B.I.$$iINSPIRE-00326936$$uIllinois U., Chicago
000030448 245__ $$aCharged and strange hadron elliptic flow in Cu+Cu collisions at $\sqrt{s_{NN}}$ = 62.4 and 200 GeV
000030448 246__ $$9arXiv$$aCharged and strange hadron elliptic flow in Cu+Cu collisions at $\sqrt{s_{NN}}$ = 62.4 and 200 GeV
000030448 269__ $$c2010-01
000030448 300__ $$a18
000030448 520__ $$9arXiv$$aWe present the results of an elliptic flow analysis of Cu+Cu collisions recorded with the STAR detector at 62.4 and 200GeV. Elliptic flow as a function of transverse momentum is reported for different collision centralities for charged hadrons and strangeness containing hadrons $K_{S}^{0}$, $\Lambda$, $\Xi$, $\phi$ in the midrapidity region $|eta|<1.0$. Significant reduction in systematic uncertainty of the measurement due to non-flow effects has been achieved by correlating particles at midrapidity, $|\eta|<1.0$, with those at forward rapidity, $2.5<|\eta|<4.0$. We also present azimuthal correlations in p+p collisions at 200 GeV to help estimating non-flow effects. To study the system-size dependence of elliptic flow, we present a detailed comparison with previously published results from Au+Au collisions at 200 GeV. We observe that $v_{2}$($p_{T}$) of strange hadrons has similar scaling properties as were first observed in Au+Au collisions, i.e.: (i) at low transverse momenta, $p_T<2GeV/c$, $v_{2}$ scales with transverse kinetic energy, $m_{T}-m$, and (ii) at intermediate $p_T$, $2<p_T<4GeV/c$, it scales with the number of constituent quarks, $n_q$. We have found that ideal hydrodynamic calculations fail to reproduce the centrality dependence of $v_{2}$($p_{T}$) for $K_{S}^{0}$ and $\Lambda$. Eccentricity scaled $v_2$ values, $v_{2}/\epsilon$, are larger in more central collisions, suggesting stronger collective flow develops in more central collisions. The comparison with Au+Au collisions which go further in density shows $v_{2}/\epsilon$ depend on the system size, number of participants $N_{part}$. This indicates that the ideal hydrodynamic limit is not reached in Cu+Cu collisions, presumably because the assumption of thermalization is not attained.
000030448 65017 $$2INSPIRE$$aExperiment-Nucl
000030448 6507_ $$2PACS$$a25.75.Ld
000030448 6507_ $$2PACS$$a25.75.Dw
000030448 690C_ $$2INSPIRE$$aPublished
000030448 693__ $$eBNL-RHIC-STAR
000030448 695__ $$2INSPIRE$$aheavy ion: scattering
000030448 695__ $$2INSPIRE$$acopper
000030448 695__ $$2INSPIRE$$acharged particle: elliptic flow
000030448 695__ $$2INSPIRE$$acopper
000030448 695__ $$2INSPIRE$$astrange particle: elliptic flow
000030448 695__ $$2INSPIRE$$afermion number
000030448 695__ $$2INSPIRE$$aparticle flow: collective phenomena
000030448 695__ $$2INSPIRE$$atransverse momentum: dependence
000030448 695__ $$2INSPIRE$$aimpact parameter: dependence
000030448 695__ $$2INSPIRE$$ahydrodynamics
000030448 695__ $$2INSPIRE$$aangular correlation
000030448 695__ $$2INSPIRE$$arapidity: correlation
000030448 695__ $$2INSPIRE$$aSTAR
000030448 695__ $$2INSPIRE$$ascaling
000030448 695__ $$2INSPIRE$$aexperimental results
000030448 695__ $$2INSPIRE$$aBrookhaven RHIC Coll
000030448 695__ $$2INSPIRE$$a62.4: 200.0 GeV-cms/nucleon
000030448 700__ $$aAggarwal, M.M.$$iINSPIRE-00180711$$uPanjab U.
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000030448 700__ $$aBellwied, R.$$iINSPIRE-00180735$$uWayne State U.
000030448 700__ $$aBetancourt, M.J.$$iINSPIRE-00326740$$uMIT
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000030448 700__ $$aBhati, A.K.$$iINSPIRE-00180755$$uPanjab U.
000030448 700__ $$aBichsel, H.$$iINSPIRE-00066925$$uWashington U., Seattle
000030448 700__ $$aBielcik, J.$$iINSPIRE-00180768$$uPrague, Tech. U.
000030448 700__ $$aBielcikova, J.$$iINSPIRE-00180776$$uRez, Nucl. Phys. Inst.
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000030448 700__ $$aBrandin, A.V.$$iINSPIRE-00180792$$uMoscow Phys. Eng. Inst.
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000030448 700__ $$aCalderon de la Barca Sanchez, M.$$iINSPIRE-00050487$$uUC, Davis
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000030448 700__ $$aCervantes, M.C.$$iINSPIRE-00180898$$uTexas A-M
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000030448 700__ $$aChaloupka, P.$$iINSPIRE-00180911$$uRez, Nucl. Phys. Inst.
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000030448 700__ $$aCherney, M.$$iINSPIRE-00184613$$uCreighton U.
000030448 700__ $$aChikanian, A.$$iINSPIRE-00180978$$uYale U.
000030448 700__ $$aChoi, K.E.$$iINSPIRE-00180982$$uPusan Natl. U.
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000030448 700__ $$aChung, P.$$iINSPIRE-00181002$$uRez, Nucl. Phys. Inst.
000030448 700__ $$aClarke, R.F.$$iINSPIRE-00181013$$uTexas A-M
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000030448 700__ $$aGuertin, S.M.$$iINSPIRE-00181726$$uUCLA
000030448 700__ $$aGupta, A.$$iINSPIRE-00181730$$uJammu U.
000030448 700__ $$aGupta, N.$$iINSPIRE-00181741$$uJammu U.
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000030448 700__ $$aHoffmann, G.W.$$iINSPIRE-00039591$$uTexas U.
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000030448 700__ $$aJakl, P.$$iINSPIRE-00181895$$uRez, Nucl. Phys. Inst.
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000030448 700__ $$aKajimoto, K.$$iINSPIRE-00181963$$uTexas U.
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000030448 700__ $$aKapitan, J.$$iINSPIRE-00181991$$uRez, Nucl. Phys. Inst.
000030448 700__ $$aKauder, K.$$iINSPIRE-00182003$$uIllinois U., Chicago
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000030448 700__ $$aKotchenda, L.$$iINSPIRE-00182120$$uMoscow Phys. Eng. Inst.
000030448 700__ $$aKouchpil, V.$$iINSPIRE-00182134$$uRez, Nucl. Phys. Inst.
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000030448 700__ $$aMinaev, N.G.$$iINSPIRE-00182524$$uSerpukhov, IHEP
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000030448 700__ $$aPawlak, T.$$iINSPIRE-00182716$$uWarsaw U. of Tech.
000030448 700__ $$aPeitzmann, T.$$iINSPIRE-00182726$$uNIKHEF, Amsterdam
000030448 700__ $$aPerevoztchikov, V.$$iINSPIRE-00115612$$uBrookhaven
000030448 700__ $$aPerkins, C.$$iINSPIRE-00182738$$uUC, Berkeley
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000030448 700__ $$aPhatak, S.C.$$iINSPIRE-00182755$$uBhubaneswar, Inst. Phys.
000030448 700__ $$aPile, P.$$iINSPIRE-00182768$$uBrookhaven
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000030448 700__ $$aZoulkarneeva, Y.$$iINSPIRE-00183830$$uDubna, JINR
000030448 710__ $$gThe STAR Collaboration
000030448 773__ $$a10.1103/PhysRevC.81.044902$$c044902$$pPhys.Rev.$$vC81$$y2010
000030448 8564_ $$uhttp://inspirebeta.net/record/843985/files/AA_pp.png$$y00001 (Color online) Charged hadron azimuthal correlations as a function of \pt in \sqrtsNN = 200 GeV 60\% most central \cucu collisions (closed squares) compared to those from \sqrtsNN = 200 GeV \pp collisions (open squares). Flow vector calculated from (a) TPCtracks, (b) FTPC tracks. The error bars are shown only for the statistical uncertainties.
000030448 8564_ $$uhttp://inspirebeta.net/record/843985/files/AuCu_cent_MSH.png$$y00012 (Color online) Centrality dependence of \vtwo scaled by number of quarks and participant eccentricity ($v_2/$($n_q \times$\eparttwos)) for \ks(left) and \lam(right) as a function of ($m_T - m$)/$n_q$ in $0-10$\%, $10-40$\% and $40-80$\% \auau collisions (open symbols)~\cite{star_v2cen} and $0-20$\% and $20-60$\% \cucu collisions (solid symbols) at \sqrtsNN = 200 GeV. Curves are the results of $n_q$-scaling fits from Eq.~(\ref{Equation:Fitv2}) normalized by \eparttwo to combined \ks and \lam for five centrality bins. At a given $p_{T}$, from top to bottom, the curves show a decreasing trend as a function of \npart.The error bars are shown only for the statistical uncertainties.
000030448 8564_ $$uhttp://inspirebeta.net/record/843985/files/AuCu_minibias.png$$y00013 (Color online) Number of quarks and participant eccentricity scaled \vtwo ($v_2/$($n_q \times$\eparttwos)) of identified particles as a function of ($m_T - m$)/$n_q$ in $0-80$\% \auau collisions (open symbols)~\cite{star_v2cen} and $0-60$\% \cucu collisions (closed symbols) at \sqrtsNN = 200 GeV. Circles, squares and triangles represent the data for \kss, $\Lambda$ and $\Xi$,respectively. The error bars are shown only for the statistical uncertainties.
000030448 8564_ $$uhttp://inspirebeta.net/record/843985/files/Integral_v2.png$$y00005 (Color online) Charged hadron \vtwo integrated over \pt and $\eta$ vs. centrality for the various methods described in thetext in \sqrtsNN = 200 GeV and 62.4 GeV \cucu collisions. The error bars are shown only for the statistical uncertainties.
000030448 8564_ $$uhttp://inspirebeta.net/record/843985/files/pid200cucu.png$$y00000 (Color online) Invariant mass distributions for (a) \ks ($1.2 < p_{T} < 1.4\ \GeVc$), (b) $\phi$ ($1.0 < p_{T} < 2.0\ \GeVc$), (c) $\Lambda$ ($1.4 < p_{T} < 1.6\ \GeVc$) and (d) $\Xi$ ($1.25 < p_{T} < 1.75\ \GeVc$) in \sqrtsNN = 200 GeV \cucu 60\% most central collisions. The solid curves represent the fits to the invariant mass distributions: Gaussians plus fourth-order polynomials for \kss, $\Lambda$ and $\Xi$, Breit-Wigner plus a linear function for $\phi$. The dotted curves are the estimated backgrounds: the fourth order polynomials for \ks and $\Lambda$, a linear function for $\phi$, and a rotation method described in the text for $\Xi$. For clarity, the invariant mass distributions for \ks, $\Lambda$, $\phi$ and $\Xi$ are scaled by 1/50 000, 1/130 000, 1/5 000 and 1/8 000, respectively.The error bars are shown only for the statistical uncertainties.
000030448 8564_ $$uhttp://inspirebeta.net/record/843985/files/v262GeV200GeVv2.png$$y00007 (Color online) (a) Charged hadron $v_2$ as a function of \pt in \cucu collisions. The results from \sqrtsNN = 200 GeV and 62.4 GeV are presented by open symbols and closed symbols, respectively. (b) Ratios of the $v_2$($p_T$) from \sqrtsNN = 62.4 GeVto 200 GeV. The error bars are shown only for the statistical uncertainties.
000030448 8564_ $$uhttp://inspirebeta.net/record/843985/files/v2Eccchgpt.png$$y00011 (Color online) $v_2$ scaled by participant eccentricity as a function of $p_T$ in \sqrtsNN =200 and 62.4 GeV \cucu collisions. The error bars are shown only for the statistical uncertainties.
000030448 8564_ $$uhttp://inspirebeta.net/record/843985/files/v2NqPtMt.png$$y00010 (Color online) \vtwo/\nq versus \pts/\nq (panels (a1)-(a3)) and (\kets)/\nq (panels (b1)-(b3)), where \nq is the number of constituent quarks in the hadron. The parametrization Eq.~(\ref{Equation:Fitv2}) fitted to the data is shown as the dashed curves. Alldata are from \sqrtsNN = 200 GeV \cucu collisions. The error bars are shown only for the statistical uncertainties.
000030448 8564_ $$uhttp://inspirebeta.net/record/843985/files/v2PtMt.png$$y00008 (Color online) \vtwo of \ks (open circles), $\Lambda$ ( solid squares), $\Xi$ (solid triangles) and $\phi$ (open stars) as a function of \pt for (a1) $0-60\%$, (a2) $0-20\%$, (a3) $20-60\%$ and as a function of \ket~for (b1) $0-60\%$, (b2) $0-20\%$, (b3) $20-60\%$. For comparisons, the results from ideal hydrodynamic calculations~\cite{pasirev06,pasi08} are also shown. At a given $p_T$, from top to bottom, the curves represent $\pi$, $K$, $p$, $\phi$, $\Lambda$, $\Xi$ and $\Omega$. When \pt is converted to \kets, this mass hierarchy is reversed in the model results. Alldata are from \sqrtsNN = 200 GeV \cucu collisions. The error bars are shown only for the statistical uncertainties. : (Color online) Same as Fig.~\ref{v2PtMt}~(a1) and (b1), but expanded for the low \pts~and \ket regions. The data points with large errors have not been plotted. At a given $p_T$, from top to bottom, the curves represent the ideal hydrodynamic calculations for $\pi$, $K$, $p$, $\phi$, $\Lambda$, $\Xi$ and $\Omega$~\cite{pasirev06,pasi08}. When \pt is converted to \kets, this mass hierarchy is reversed in the model results. All data are from $0-60\%$ \cucu collisions at \sqrtsNN = 200 GeV.The error bars are shown only for the statistical uncertainties.
000030448 8564_ $$uhttp://inspirebeta.net/record/843985/files/v2PtMtZoomin.png$$y00009 (Color online) Same as Fig.~\ref{v2PtMt}~(a1) and (b1), but expanded for the low \pts~and \ket regions. The data points with large errors have not been plotted. At a given $p_T$, from top to bottom, the curves represent the ideal hydrodynamic calculations for $\pi$, $K$, $p$, $\phi$, $\Lambda$, $\Xi$ and $\Omega$~\cite{pasirev06,pasi08}. When \pt is converted to \kets, this mass hierarchy is reversed in the model results. All data are from $0-60\%$ \cucu collisions at \sqrtsNN = 200 GeV.The error bars are shown only for the statistical uncertainties.
000030448 8564_ $$uhttp://inspirebeta.net/record/843985/files/v2Ratiochgcen.png$$y00004 Ratios of $v_{2}\{AA-pp, \rm FTPC\}$/$v_{2}\{\rm FTPC\}$ for charged hadron as function of \pt in \sqrtsNN = 200 GeV \cucu collisions for centrality bins: (a) $50-60\%$, (b) $40-50\%$, (c) $30-40\%$, (d) $20-30\%$, (e) $10-20\%$ and (f) $0-10\%$. The percentages refer to fraction ofmost central events.
000030448 8564_ $$uhttp://inspirebeta.net/record/843985/files/v2chgcen.png$$y00003 (Color online) Charged hadron $v_{2}\{\rm FTPC\}$ (closed circles) and $v_{2}\{AA-pp, \rm FTPC\}$ (open circles) as function of \pt in \sqrtsNN = 200 GeV \cucu collisions for centrality bins: (a) $50-60\%$, (b) $40-50\%$, (c) $30-40\%$, (d) $20-30\%$, (e) $10-20\%$ and (f) $0-10\%$. The percentages refer to fraction ofmost central events. The error bars are shown only for the statistical uncertainties.
000030448 8564_ $$uhttp://inspirebeta.net/record/843985/files/v2chgmini.png$$y00002 (Color online) (a) Charged hadron \vtwos(\pts) in \sqrtsNN = 200 GeV $0-60\%$ \cucu collisions. Open circles, closed circles, open squares and closed squares represent the results of $v_{2}$ as function of \pt measured by the TPC flow vector ($v_{2}\{\rm TPC\}$), the FTPC flow vector ($v_{2}\{\rm FTPC\}$), the TPC and FTPC flow vector with subtracting the azimuthal correlations in \pp collisions ($v_{2}\{AA-pp, \rm TPC\}$, $v_{2}\{AA-pp, \rm FTPC\}$). (b) The ratio of the results for the various methods described in (a).The error bars are shown only for the statistical uncertainties.
000030448 8564_ $$uhttp://inspirebeta.net/record/843985/files/v2chgpt.png$$y00006 (Color online) Charged hadron $v_{2}$ as function of \pt for $50-60\%$ (solid circles), $40-50\%$ (solid squares), $30-40\%$ (solid triangles), $20-30\%$ (open circles), $10-20\%$ (open squares) and $0-10\%$ (open triangles) in \sqrtsNN = 200 GeV and 62.4 GeV \cucucollisions. The error bars are shown only for the statistical uncertainties.
000030448 909CO $$ooai:jdsweb.jinr.ru:30448$$pglobal
000030448 961__ $$x2010-01-28
000030448 961__ $$c2010-05-05
000030448 970__ $$aSPIRES-8540560
000030448 980__ $$aPublished
000030448 980__ $$aarXiv
000030448 980__ $$aCiteable
000030448 980__ $$aCORE
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