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@ARTICLE{Acharya:363835,
      author       = {Acharya, Shreyasi and others},
      title        = {{R}apidity dependence of antideuteron coalescence in pp
                      collisions at $\sqrt{s}$ = 13 {T}e{V} with {ALICE}},
      journal      = {Physics letters / B},
      volume       = {860},
      issn         = {0031-9163},
      address      = {Amsterdam},
      publisher    = {North-Holland Publ.},
      reportid     = {GSI-2026-00045, arXiv:2407.10527. CERN-EP-2024-187},
      pages        = {139191},
      year         = {2025},
      note         = {Phys. Lett. B 860 (2025) 139191. 23 pages, 4 captioned
                      figures, 1 table, authors from page 17, published version,
                      figures at
                      http://alice-publications.web.cern.ch/node/11236SCAOP3
                      ccby4.0 "Funded by SCOAP³. This is an open access article
                      under the CC BY license
                      (http://creativecommons.org/licenses/by/4.0/)."},
      abstract     = {The production yields of antideuterons and antiprotons are
                      measured in pp collisions at a center-of-mass energy of
                      $\sqrt{s}$ = 13 TeV, as a function of transverse momentum
                      ($p_T$) and rapidity (y), for the first time
                      rapidity-differentially up to |y| = 0.7. The measured
                      spectra are used to study the $p_T$ and rapidity dependence
                      of the coalescence parameter $B_2$, which quantifies the
                      coalescence probability of antideuterons. The $p_T$ and
                      rapidity dependence of the obtained $B_2$ is extrapolated
                      for $p_T$ > 1.7 GeV/c and |y| > 0.7 using the
                      phenomenological antideuteron production model implemented
                      in Pythia 8.3 as well as a baryon coalescence afterburner
                      model based on EPOS 3. Such measurements are of interest to
                      the astrophysics community, since they can be used for the
                      calculation of the flux of antinuclei from cosmic rays, in
                      combination with coalescence models.},
      cin          = {ALI / DTL / CIT / EXM / ALICE@CERN},
      ddc          = {530},
      cid          = {I:(DE-Ds200)ALI-20080822OR105 /
                      I:(DE-Ds200)DTL-20051214OR031 /
                      I:(DE-Ds200)CIT-20110310OR121 /
                      I:(DE-Ds200)EXM-20080818OR100 / I:(DE-Ds200)Coll-CERN-ALICE},
      pnm          = {612 - Cosmic Matter in the Laboratory (POF4-612) / HGS-HIRe
                      - HGS-HIRe for FAIR (HGS-HIRe) / SUC-GSI-Heidelberg -
                      Strategic university cooperation GSI-U Heidelberg
                      (SUC-GSI-HE) / SUC-GSI-Frankfurt - Strategic university
                      cooperation GSI-U Frankfurt/M (SUC-GSI-FR) /
                      SUC-GSI-Darmstadt - Strategic university cooperation GSI-TU
                      Darmstadt (SUC-GSI-DA) / STRONG-2020 - The strong
                      interaction at the frontier of knowledge: fundamental
                      research and applications (824093)},
      pid          = {G:(DE-HGF)POF4-612 / G:(DE-Ds200)HGS-HIRe /
                      G:(DE-Ds200)SUC-GSI-HE / G:(DE-Ds200)SUC-GSI-FR /
                      G:(DE-Ds200)SUC-GSI-DA / G:(EU-Grant)824093},
      experiment   = {EXP:(DE-H253)LHC-Exp-ALICE-20150101},
      typ          = {PUB:(DE-HGF)16},
      eprint       = {2407.10527},
      howpublished = {arXiv:2407.10527},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2407.10527;\%\%$},
      UT           = {WOS:001399994700001},
      doi          = {10.1016/j.physletb.2024.139191},
      url          = {https://repository.gsi.de/record/363835},
}