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Excess of J/ y yield at very low p T in Au+Au collisions at = 200 GeV and U+U collisions at = 193 GeV with STAR Wangmei Zha for the STAR Collaboration University of Science and Technology of China W. Zha etal.,


  1. Excess of J/ y yield at very low p T in Au+Au collisions at 𝑑 𝑂𝑂 = 200 GeV and U+U collisions at 𝑑 𝑂𝑂 = 193 GeV with STAR Wangmei Zha for the STAR Collaboration University of Science and Technology of China W. Zha etal., arXiv: 1705.01460 The 21 st Particles & Nuclei International Conference 1-5 September, IHEP, Beijing, China Wangmei Zha, PANIC2017, IHEP, Beijing, 1 China

  2. J/ y production and modification in hadronic A+A collisions οƒ˜ Hot medium effects: οƒΌ Color Screening - β€œSmoking gun” signature for QGP formation οƒΌ Regeneration -Recombination of charm quarks οƒ˜ Cold Nuclear Matter effects: οƒΌ PDF modification in nucleus STAR Collab., Phys. Lett. B 771 (2017) 13 οƒΌ Initial state energy loss οƒΌ Cronin effect οƒΌ Nuclear absorption οƒ˜ Final state effect: οƒΌ Dissociation by co-mover X. Zhao etal., Phys. Rev. C 82 {2010) 064905 The interplay of these effects can R AA = explain the results from SPS to LHC! Wangmei Zha, PANIC2017, IHEP, Beijing, China 2

  3. Excess of J/ y production at very low p T with ALICE οƒΌ Significant enhancement of J/ y yield observed in p T interval 0 – 0.3 GeV/c for peripheral collisions (50 – 90%). οƒΌ Can not be described by hadronic production modified by the hot ALICE Collab., Phys. Rev. Lett. 116 (2016) 222301 medium or cold nuclear matter effects! οƒΌ Originate from coherent photon- nucleus interactions? οƒ˜ Measurement of J/ y yield at very low p T in hadronic collisions (U+U and Au+Au): οƒ˜ Enhancement of J/ y yield at very low p T ? οƒ˜ If so, what are the properties and the origin of the excess? οƒ˜ p T , centrality and system size dependence of the excess; t distribution. Wangmei Zha, PANIC2017, IHEP, Beijing, China 3

  4. Introduction to photon interactions in A+A C.A. Bertulani etal., Ann. Rev. Nucl. Part. Sci 55 (2005) 271 = + V= r , w , f , J/ y Photon-photon Photon-nucleus Electromagnetic interaction interactions interactions  The large flux of quasi-real photons makes a hadron collider also a photon collider!  Photon-nucleus interactions: οƒ˜ Coherent: emitted photon interacts with the entire target nucleus. οƒ˜ Incoherent: emitted photon interacts with nucleon or parton individually. Wangmei Zha, PANIC2017, IHEP, Beijing, China 4

  5. Features of coherent photon-nucleus interaction  Coherently: οƒΌ Both nuclei remain intact οƒΌ Photon/Pomeron wavelength l = w/o interference β„Ž w/ interference π‘ž > 𝑆 𝐡 (nucleus radius) οƒΌ p T < β„Ž/𝑆 𝐡 ~30 MeV/c for heavy ions οƒΌ Strong couplings ( π‘Žπ›½ 𝐹𝑁 ~ 0.6) οƒ  y = 0 large cross sections  Interference: οƒΌ Two indistinguishable processes (photon from A 1 or A 2 ) οƒΌ Vector meson οƒ  opposite signs in amplitude of production οƒΌ Significant destructive interference S.R. Klein and J. Nystrand, Phys. Rev. Lett. 84 (2000) 2330 for p T << 1/<b> Wangmei Zha, PANIC2017, IHEP, Beijing, China 5

  6. J/ y hadronic production versus photoproduction  J/ y can be produced via strong and electromagnetic interactions.  The strong interactions can obscure the electromagnetic interactions  Study the electromagnetic process in Ultra-Peripheral Collisions (UPC) οƒΌ UPC conditions (b > 2R A ): no hadronic interactions Hadronic collisions: UPC collisions: J/ y hadronic production J/ y photoproduction and modification Wangmei Zha, PANIC2017, IHEP, Beijing, China 6

  7. The STAR detector οƒ˜ Large acceptance: | h | < 1, 0 < f < 2Ο€ οƒ˜ Time Projection Chamber (TPC) – tracking, particle identification, momentum οƒ˜ Time of Flight detector (TOF) – particle identification οƒ˜ Barrel ElectroMagnetic Calorimeter (BEMC) – electron identification, triggering Wangmei Zha, PANIC2017, IHEP, Beijing, China 7

  8. Electron identification 1/ b distribution for electrons and hadrons from TOF Normalized dE/dx (n s e ) distribution before and after TOF cuts STAR preliminary p/E distribution for electrons and hadrons from BEMC STAR preliminary Normalized counts STAR Collab., Phys. Rev. C 92 (2015) 24912 Wangmei Zha, PANIC2017, IHEP, Beijing, China 8

  9. J/ y signal Centrality: 40 – 80% The signal is extracted by subtracting the mixed event background from the unlike-sign pairs. Good signal over background ratio! Wangmei Zha, PANIC2017, IHEP, Beijing, China 9

  10. J/ y invariant yield in Au+Au and U+U collisions 40 – 60% 60 – 80% Function to describe hadronic production: 𝑒 2 𝑂 1 = 𝑏 Γ— 2 ) π‘œ π‘ž π‘ˆ π‘’π‘ž π‘ˆ (1 + 𝑐 2 π‘ž π‘ˆ οƒ˜ Significant enhancement of J/ y yield observed at p T interval 0 – 0.2 GeV/c 20 – 40% for peripheral collisions (40 – 80 %)! οƒ˜ The yield of J/ y at very low p T in Au+Au is similar to that in U+U within uncertainties. Wangmei Zha, PANIC2017, IHEP, Beijing, China 10

  11. J/ y yield at very low p T versus centrality 30 – 40% οƒΌ No significant centrality dependence of the excess yield! οƒΌ Low p T J/ y from hadronic production is expected to increase dramatically with N part . οƒΌ No significant difference between Au+Au and U+U collisions. Wangmei Zha, PANIC2017, IHEP, Beijing, China 11

  12. J/ y dN/dt distribution for 40-80% Au+Au collisions Au+Au Au+Au 200 GeV 200 GeV UPC r 0 οƒΌ Similar structure to that in UPC case! οƒΌ Indication of interference! STAR Collab., Phys. Rev. C 77 (2008) 4910 ρ 0 cross-section as a function of the οƒΌ Interference shape from calculation for UPC case 2 ) momentum transfer squared ( 𝑒 β‰ˆ π‘ž π‘ˆ S.R. Klein and J. Nystrand, Phys. Rev. Lett. 84 (2000) 2330 οƒΌ Similar slope parameter! from STAR UPC measurements. οƒΌ Slope from STARLIGHT prediction in UPC case  The slope from the exponential – 196 (GeV/c) -2 Slope w/o the first point: 199 Β± 31(GeV/c) -2 οƒΌ fit reflects the density profile of c 2 /𝑂𝐸𝐺 = 1.7/2 the target. οƒΌ Slope with the first point: 164 Β± 24(GeV/c) -2 c 2 /𝑂𝐸𝐺 = 5.9/3 Wangmei Zha, PANIC2017, IHEP, Beijing, China 12

  13. J/ y p+p baseline extraction from world-wide data οƒΌ The scaled rapidity and p T distributions follow a universal trend. οƒΌ p+p baseline at very low p T is interpolated from the world- z T = p T /<p T > wide experimental data. W. Zha etal., Phys. Rev. C93 (2016) 024919 Wangmei Zha, PANIC2017, IHEP, Beijing, China 13

  14. J/ y R AA for Au+Au and U+U collisions 60 – 80% 40 – 60%  R AA ~ 20 in 60 – 80% centrality at p T interval 0 – 0.1 20 – 40% GeV/c  R AA ~ 4 for 40 – 60% centrality at p T interval 0 – 0.1 GeV/c Wangmei Zha, PANIC2017, IHEP, Beijing, China 14

  15. Model for J/ y photoproduction in hadronic collisions Photon emitter and target OR nucleus spectator W. Zha etal., arXiv: 1705.01460 Photon emitter Target Nucleus Nucleus (1) The density profile of Nucleus Spectator (2) spectators is from optical Spectator Nucleus (3) Glauber calculations! Spectator Spectator (4) Incoherent contribution, cold nuclear and hot medium effects are not included in the calculations! Wangmei Zha, PANIC2017, IHEP, Beijing, China 15

  16. Model calculations with different scenarios W. Zha etal., arXiv: 1705.01460 Nucleus + Nucleus οƒΌ All four scenarios describe data well in peripheral collisions (60-80%)! οƒΌ Different scenarios have different trends toward central collisions! οƒΌ The data favor β€œNucleus + Spectator” and β€œSpectator + Nucleus”. οƒΌ To distinguish the different scenarios, measurements in central collisions are needed! οƒΌ Calculations based on the β€œNucleus + Nucleus” scenario describe the t distribution! οƒΌ The differences between different scenarios in t distributions are negligible in 40-80% centrality class. Wangmei Zha, PANIC2017, IHEP, Beijing, China 16

  17. Summary οƒ˜ Significant excess of J/ y yield at p T interval 0 – 0.2 GeV/c is observed in peripheral Au+Au and U+U collisions (40 – 80%). οƒ˜ The excess has no significant centrality dependence (40 – 80%) within uncertainties, which is different from the expectation from hadronic production. οƒ˜ The properties of the excess are consistent with coherent photon-nucleus interactions. οƒΌ Similar dN/dt distribution to that in UPC case. οƒΌ Indication of interference at p T interval 0 – 0.03 GeV/c. οƒΌ The extracted nuclear form factor slope is consistent with nucleus size. οƒ˜ A theoretical calculation based on coherent photoproduction scenario can qualitatively describe the excess. Wangmei Zha, PANIC2017, IHEP, Beijing, China 17

  18. Future directions: more differentially ----p T shape with different scenarios Nucleus+Spectator Nucleus+Nucleus Spectator+Spectator Spectator+Nucleus οƒΌ The p T shape is very sensitive to the target! οƒΌ If the target is spectator, the p T shape has significant centrality dependence! Wangmei Zha, PANIC2017, IHEP, Beijing, China 18

  19. Production versus f (relative to reaction plane) Phys. Rev. C 77 77 (2008) 54901 οƒΌ Sensitive to the target! οƒΌ Large v 2 and sizeable v 4 will be observed if the target is spectator! οƒΌ V 2 increase dramatically toward central collisions! οƒΌ Probe of initial geometry of the overlap region! Wangmei Zha, PANIC2017, IHEP, Beijing, China 19

  20. p T shape with interference οƒΌ Dramatically change the p T spectra! οƒΌ Different interference pattern in different centrality! οƒΌ The effect is relative small with spectator coupling! Wangmei Zha, PANIC2017, IHEP, Beijing, China 20

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