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@ARTICLE{Steinheimer:46037,
      author       = {Steinheimer, J. and Gudima, K. and Botvina, A. and
                      Mishustin, I. and Bleicher, M. and Stöcker, Horst},
      title        = {{H}ypernuclei, dibaryon and antinuclei production in high
                      energy heavy ion collisions: {T}hermal production vs.
                      coalescence},
      journal      = {Physics letters / B},
      volume       = {714},
      number       = {1},
      issn         = {0370-2693},
      address      = {Amsterdam},
      publisher    = {North-Holland Publ.},
      reportid     = {GSI-2013-00016},
      pages        = {85 - 91},
      year         = {2012},
      note         = {9 pages, 8 figures and 2 tables, version accepted by PLB},
      abstract     = {We study the production of (hyper-)nuclei and di-baryons in
                      most central heavy Ion collisions at energies of
                      $E_{lab}=1-160 A$ GeV. In particular we are interested in
                      clusters produced from the hot and dense fireball. The
                      formation rate of strange and non-strange clusters is
                      estimated by assuming thermal production from the
                      intermediate phase of the UrQMD-hydro hybrid model and
                      alternatively by the coalescence mechanism from a hadronic
                      cascade model. Both model types are compared in detail. For
                      most energies we find that both approaches agree in their
                      predictions for the yields of the clusters. Only for very
                      low beam energies, and for di-baryons including $Xi$'s, we
                      observe considerable differences. We also study the
                      production of anti-matter clusters up to top RHIC energies
                      and show that the observation of anti-$^4He$ and even
                      anti-$^4_{Lambda}He$ is feasible. We have found a
                      considerable qualitative difference in the energy dependence
                      of the strangeness population factor $R_H$ when comparing
                      the thermal production with the coalescence results.},
      cin          = {THE / WGF},
      ddc          = {530},
      cid          = {I:(DE-Ds200)THE-20051214OR028 /
                      I:(DE-Ds200)WGF-20100910OR011},
      pnm          = {532 - Nuclear and Quark Gluon Matter (NQM) (POF2-532)},
      pid          = {G:(DE-HGF)POF2-532},
      typ          = {PUB:(DE-HGF)25},
      eprint       = {1203.2547},
      howpublished = {arXiv:1203.2547},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:1203.2547;\%\%$},
      doi          = {10.1016/j.physletb.2012.06.069},
      url          = {https://repository.gsi.de/record/46037},
}