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Multi-charmed and singled charmed hadrons from coalescence: yields and ratios in different collision systems at LHC
We study the production of charmed and multi-charmed hadrons in ultra-relativistic Heavy Ion Collisions coupling the transport approach for charm dynamics in the medium to an hybrid hadronization model of coalescence plus fragmentation. In this paper, we mainly discuss the particle yields for single...
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Published in: | The European physical journal. C, Particles and fields Particles and fields, 2024-03, Vol.84 (3), p.228-13, Article 228 |
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Main Authors: | , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | We study the production of charmed and multi-charmed hadrons in ultra-relativistic Heavy Ion Collisions coupling the transport approach for charm dynamics in the medium to an hybrid hadronization model of coalescence plus fragmentation. In this paper, we mainly discuss the particle yields for single charmed and multi-charmed baryons focusing mainly on the production of
Ξ
cc
and
Ω
ccc
. We provide first predictions for
PbPb
collision in
0
-
10
%
centrality class and then we explore the system size dependence through
KrKr
, to
ArAr
and
OO
collisions, planned within the ALICE3 experiment. In these cases, a monotonic behavior for the yields emerges which can be tested in future experimental data. We found about three order of magnitude increase in the production of
Ω
ccc
in
PbPb
collisions compared with the yield in small collision systems like
OO
collisions. Furthermore, we investigate the effects on the
Ω
ccc
particle yield and spectra coming from the modification of the charm quark distribution due to the different size of the collision systems also comparing it to the case of thermalized charm distributions. These results suggest that observation on the
Ω
ccc
spectra and their evolution across system size can give novel information about the partial thermalization of the charm quark distribution as well as to its wave function width. Furthermore, we find that the
Ω
ccc
/
D
0
ratio is an observable more sensitive with respect to
Λ
c
/
D
0
, this ratio is predicted to span over two order of magnitude from large to small systems. |
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ISSN: | 1434-6052 1434-6044 1434-6052 |
DOI: | 10.1140/epjc/s10052-024-12571-6 |