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Richard Bindel, UMDDivision of Nuclear Physics, Maui, 2005 System Size and Energy Dependence of Elliptical Flow Richard Bindel University of Maryland For.

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Presentation on theme: "Richard Bindel, UMDDivision of Nuclear Physics, Maui, 2005 System Size and Energy Dependence of Elliptical Flow Richard Bindel University of Maryland For."— Presentation transcript:

1 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 2005 System Size and Energy Dependence of Elliptical Flow Richard Bindel University of Maryland For the collaboration Division of Nuclear Physics, Maui September 19th, 2005

2 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 20052 Collaboration (Aug 2005)

3 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 20053 Motivation For Studying Flow Reaction plane x z y M. Kaneta Flow probes the very early thermalization of the system Elliptic flow as a function of: Energy Centrality Pseudorapidity Momentum Can be used to constrain theory.

4 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 20054 Two Flow Measurement Methods Hit Based MethodTrack Based Method

5 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 20055 Motivation for Comparing Species Mid-central AuAu collision Central CuCu collision Two similar system sizes! roughly same number of participants

6 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 20056 Cu+Cu Preliminary 3-6%, N part = 100 Au+Au 35-40%, N part = 99 Some observables scale with number of participants Similar dN/d  Motivation for Comparing Species Mid-central AuAu collision Central CuCu collision Two similar system sizes! 200 GeV roughly same number of participants

7 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 20057 Cu+Cu Preliminary 3-6%, N part = 100 Au+Au 35-40%, N part = 99 200 GeV Some observables scale with number of participants Similar dN/d  Motivation for Comparing Species Mid-central AuAu collision Central CuCu collision Two similar system sizes! We expect flow to depend on geometry! Two similar system sizes! roughly same number of participants

8 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 20058 Cu+Cu Preliminary 3-6%, N part = 100 Au+Au 35-40%, N part = 99 200 GeV Some observables scale with number of participants Similar dN/d  Motivation for Comparing Species Mid-central AuAu collision Central CuCu collision Two similar system sizes! We expect flow to depend on geometry! Two similar system sizes! roughly same number of participants Elliptical Circular Using two species lets us change the geometry while holding the number of participants constant

9 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 20059 Eccentricity: A measure of “Geometry” Mid-central AuAu collision Central CuCu collision Elliptical Circular We need a way to quantify the geometry of the participating nucleons The shape is characterized by the eccentricity (  )

10 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200510 Eccentricity: A measure of “Geometry” Nucleus A Nucleus B Participant Nucleons A model of a AuAu collision:

11 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200511 Eccentricity: A measure of “Geometry” Nucleus A Nucleus B Participant Nucleons A model of a AuAu collision: b Using the impact parameter as the x-axis, we define the standard eccentricity using the widths of the distribution in the x and y directions

12 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200512 Eccentricity: A measure of “Geometry” Nucleus A Nucleus B Participant Nucleons A model of a AuAu collision: b Using the impact parameter as the x-axis, we define the standard eccentricity using the widths of the distribution in the x and y directions y2y2 x2x2

13 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200513 Au+Au 19.6 GeV62.4 GeV130 GeV 200 GeV Cu+Cu 0.05 Au+Au: PRL 94 122303 (2005) preliminary PHOBOS Sizable v 2 for Cu+Cu The Phobos Elliptic Flow Data Set from 0% to 40% centrality

14 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200514 preliminary PHOBOS 200 GeV h ± Statistical errors only Cu+Cu preliminary Au+Au PHOBOS 200 GeV Hit Based Statistical errors only The Data: Something’s Amiss… Elliptic flow is high even for the most central bin in Cu+Cu How does it relate to the eccentricity? |  | < 1

15 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200515 preliminary PHOBOS 200 GeV h ± Statistical errors only Cu+Cu preliminary Au+Au PHOBOS 200 GeV Hit Based Statistical errors only For CuCu, the eccentricity drops to zero by N Part of 100 The Data: Something’s Amiss… |  | < 1

16 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200516 preliminary PHOBOS 200 Gave h ± Statistical errors only Cu+Cu preliminary Au+Au PHOBOS 200 GeV Statistical errors only v 2 near mid-rapidity The Data: Something’s Amiss… Cu+Cu preliminary Au+Au PHOBOS 200 GeV Dividing by the eccentricity shows no connection between the two species. |  | < 1

17 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200517 The Data: Something’s Amiss… What went wrong? We reexamine our definition of eccentricity

18 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200518 Reexamining Eccentricity Eccentricity is not directly measurable We use a Glauber model to relate eccentricity to our N Part bins. What goes into making this plot…?

19 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200519 Glauber collisions are modeled over a range of impact parameters and are sorted by the number of participants. Reexamining Eccentricity An eccentricity distribution is built up for each N Part The black line shows the average eccentricity AuAu AuAu collisions with same N Part

20 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200520 Reexamining Eccentricity Au-Au Cu-Cu When we examine the eccentricity distribution for CuCu, it looks much broader than AuAu Also, notice that there are many more events with negative eccentricity.

21 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200521 Meaning of Negative Eccentricity b y2y2 x2x2 Here we revisit the standard definition of eccentricity applied to a Gluaber model.

22 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200522 Meaning of Negative Eccentricity b y2y2 x2x2 Here we revisit the standard definition of eccentricity applied to a Gluaber model. Negative eccentricity results when  x 2 >  y 2, apparently due to fluctuations in the positions of the nucleons. Because of its smaller size, CuCu is more susceptible to fluctuations

23 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200523 Redefining Eccentricity Nucleus 1 Nucleus 2 Participant Region x y b One reasonable method is to realign the coordinate system to maximize the ellipsoidal shape (a principal axis transformation) “Participant” eccentricity Opposed to “standard” eccentricity

24 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200524 Standard and Participant Eccentricity Au-Au Cu-Cu Mean eccentricity shown in black Standard Eccentricity Participant Eccentricity

25 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200525 Fluctuations in eccentricity are important for the Cu-Cu system. Must use care in doing Au-Au to Cu-Cu flow comparisons. Eccentricity scaling depends on definition of eccentricity. Impact of Eccentricity Fluctuations

26 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200526 Elliptic Flow Puzzle Solved? Standard Eccentricity Cu+Cu preliminary Au+Au PHOBOS 200 GeV “Participant Eccentricity” allows v 2 scaling from Cu+Cu to Au+Au Participant Eccentricity PHOBOS 200 GeV Au+Au Cu+Cu preliminary

27 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200527 Participant Eccentricity Cu+Cu Au+Au Standard Eccentricity Cu+Cu Au+Au / scaling: STAR, PRC 66 034904 (2002) Voloshin, Poskanzer, PLB 474 27 (2000) Heiselberg, Levy, PRC 59 2716, (1999) / scaling Overlap Area Caveat: dN ch /d  corrected to dN ch /dy

28 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200528 Conclusions Phobos has continued to expand its extensive flow data set using two techniques Studying CuCu compared to AuAu allows us to vary the geometry while holding N part constant The expectation that elliptic flow scales with eccentricity continues to seem reasonable Careful consideration is needed when using eccentricity

29 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 2005 Back-up Slides

30 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200530 Limiting Fragmentation (Au+Au) 19.6 GeV62.4 GeV130 GeV200 GeV PHOBOS preliminary “Extended Longitudinal Scaling” of all longitudinal distributions  - y beam preliminary PHOBOS Au+Au 0-6% Au+Au 0-40% Au+Au 0-40% 200GeV 130GeV 62.4 GeV (prel) 19.6 GeV

31 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200531 Limiting Fragmentation (Cu+Cu) preliminary PHOBOS 62.4 GeV200 GeV ‘Extended Longitudinal Scaling’ also seen in Cu+Cu Persists from p+p to Au+Au over large range in  ′ preliminary PHOBOS  - y beam Cu+Cu 0-6% 200GeV 62.4GeV Cu+Cu 0-40%

32 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200532 Cu-Cu more like Hydro than JAM hadron string cascade model Here JAM uses a 1 fm/c formation time. Hydro (160) has kinetic freezeout temperature at 160 MeV preliminary 200 GeV Cu-Cu preliminary 200 GeV 15-25% Cu-Cu Statistical errors only Compared to JAM Model

33 Richard Bindel, UMDDivision of Nuclear Physics, Maui, 200533 PHOBOS preliminary Cu-Cu, h ± Hit based 62.4 GeV PHOBOS preliminary Cu-Cu, h ± Hit based 200 GeV Track based 200 GeV Two Flow Measurement Methods Good agreement between methods |  | < 1


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