4.5 Article

Beam energy dependence of (anti-)deuteron production in Au plus Au collisions at the BNL Relativistic Heavy Ion Collider

期刊

PHYSICAL REVIEW C
卷 99, 期 6, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevC.99.064905

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资金

  1. RHIC Operations Group at BNL
  2. RCF at BNL
  3. NERSC Center at LBNL
  4. Open Science Grid consortium
  5. Office of Nuclear Physics within the U.S. DOE Office of Science
  6. U.S. National Science Foundation
  7. Ministry of Education and Science of the Russian Federation
  8. National Natural Science Foundation of China
  9. Chinese Academy of Science
  10. Ministry of Science and Technology of China (973 Programme) [2015CB856900]
  11. Chinese Ministry of Education
  12. National Research Foundation of Korea
  13. GA of the Czech Republic
  14. MSMT of the Czech Republic
  15. Hungarian National Research, Development and Innovation Office [FK-123824]
  16. New National Excellency Programme of the Hungarian Ministry of Human Capacities [UNKP-18-4]
  17. Department of Atomic Energy of the Government of India
  18. Department of Science and Technology of the Government of India
  19. National Science Centre of Poland
  20. National Research Foundation
  21. Ministry of Science, Education and Sports of the Republic of Croatia
  22. RosAtom of Russia
  23. German Bundesministerium fur Bildung, Wissenschaft, Forschung und Technologie (BMBF)
  24. Helmholtz Association

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We report the energy dependence of mid-rapidity (anti-)deuteron production in Au+Au collisions at root s(NN) = 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4, and 200 GeV, measured by the STAR experiment at the BNL Relativistic Heavy Ion Collider. The yield of deuterons is found to be well described by the thermal model. The collision energy, centrality, and transverse momentum dependence of the coalescence parameter B-2 are discussed. We find that the values of B-2 for antideuterons are systematically lower than those for deuterons, indicating that the correlation volume of antibaryons is larger than that of baryons at root s(NN) from 19.6 to 39 GeV. In addition, values of B-2 are found to vary with collision energy and show a broad minimum around root s(NN) = 20-40 GeV, which might imply a change of the equation of state of the medium in these collisions.

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