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@ARTICLE{Vovchenko:218555,
author = {Vovchenko, Volodymyr and Dönigus, Benjamin and Stoecker,
Horst},
title = {{M}ultiplicity dependence of light nuclei production at
{LHC} energies in the canonical statistical model},
journal = {Physics letters / B B},
volume = {785},
issn = {0370-2693},
address = {Amsterdam},
publisher = {North-Holland Publ.},
reportid = {GSI-2019-00474, arXiv:1808.05245},
pages = {171 - 174},
year = {2018},
note = {This is an open access article under the CCBY license
(http://creativecommons.org/licenses/by/4.0/).
FundedbySCOAP3},
abstract = {The statistical model with exact conservation of baryon
number, electric charge, and strangeness – the Canonical
Statistical Model (CSM) – is used to analyze the
dependence of yields of light nuclei at midrapidity on
charged pion multiplicity at the LHC. The CSM calculations
are performed assuming baryon-symmetric matter, using the
recently developed Thermal-FIST package. The light
nuclei-to-proton yield ratios show a monotonic increase with
charged pion multiplicity, with a saturation at the
corresponding grand-canonical values in the
high-multiplicity limit, in good qualitative agreement with
the experimental data measured by the ALICE collaboration in
pp and Pb–Pb collisions at different centralities and
energies. Comparison with experimental data at low
multiplicities shows that exact conservation of charges
across more than one unit of rapidity and/or a chemical
freeze-out temperature which decreases with the charged pion
multiplicity improves agreement with the data.},
keywords = {pi: multiplicity (INSPIRE) / model: statistical (INSPIRE) /
multiplicity: dependence (INSPIRE) / multiplicity: low
(INSPIRE) / charge: conservation law (INSPIRE) / light
nucleus: yield (INSPIRE) / baryon number: conservation law
(INSPIRE) / light nucleus: production (INSPIRE) /
freeze-out: temperature (INSPIRE) / freeze-out: chemical
(INSPIRE) / heavy ion: scattering (INSPIRE) / CERN LHC Coll
(INSPIRE) / saturation (INSPIRE) / rapidity (INSPIRE) /
ALICE (INSPIRE)},
cin = {THE},
ddc = {530},
cid = {I:(DE-Ds200)THE-20051214OR028},
pnm = {612 - Cosmic Matter in the Laboratory (POF3-612) / OAGSI -
Open Access Publikation mit Unterstützung des GSI
Helmholtzzentrums für Schwerionenforschung (OAGSI)},
pid = {G:(DE-HGF)POF3-612 / G:(DE-Ds200)OAGSI},
typ = {PUB:(DE-HGF)16},
eprint = {1808.05245},
howpublished = {arXiv:1808.05245},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:1808.05245;\%\%$},
UT = {WOS:000447424000022},
doi = {10.1016/j.physletb.2018.08.041},
url = {https://repository.gsi.de/record/218555},
}