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Elliptic flow of $\Lambda_c^+$ in Pb--Pb collisions at $\sqrt{s_{\rm NN}}$ = 5.36 TeV in 30--50% centrality in Run 3

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Elliptic flow of $\Lambda_c^+$ in Pb--Pb collisions at $\sqrt{s_{\rm NN}}$ = 5.36  TeV in 30--50% centrality in Run 3

$v_2$ of $\Lambda_c^+$ compared with $D^0$ in Pb--Pb collisions at 5.36 TeV
Energy
5.36 TeV
System
Pb-Pb
Scope: PWG
PWG-HF (Heavy Flavour)
Figure image (.eps)
summary-lcvsd0.eps
Figure image (.pdf)
summary-lcvsd0.pdf
$v_2$ of Prompt $\Lambda_c^+$ compared with Prompt $D^0$ in Pb--Pb collisions at 5.36 TeV
Energy
5.36 TeV
System
Pb-Pb
Scope: PWG
PWG-HF (Heavy Flavour)
Figure image (.eps)
summary-promptlcvsd0.eps
Figure image (.pdf)
summary-promptlcvsd0.pdf
$v_2$  of Prompt $\Lambda_c^+$  and Prompt $D^0$ in Pb--Pb collisions at 5.36 TeV compared with models
Energy
5.36 TeV
System
Pb-Pb
Scope: PWG
PWG-HF (Heavy Flavour)
Figure image (.eps)
compare-lcvsd0-vs-model_0.eps
Figure image (.pdf)
compare-lcvsd0-vs-model_0.pdf
$v_2$  of Prompt $\Lambda_c^+$  and Prompt $D^0$ in Pb--Pb collisions at 5.36 TeV compared with tamu model
Energy
5.36 TeV
System
Pb-Pb
Scope: PWG
PWG-HF (Heavy Flavour)
Figure image (.eps)
compare-lcvsd0-vs-model_tamu.eps
Figure image (.pdf)
compare-lcvsd0-vs-model_tamu.pdf
$v_2$  of Prompt $\Lambda_c^+$  and Prompt $D^0$ in Pb--Pb collisions at 5.36 TeV compared with light flavor from published data
Energy
5.36 TeV
System
Pb-Pb
Scope: PWG
PWG-HF (Heavy Flavour)
Figure image (.eps)
compare-lcvsd0-vs-data.eps
Figure image (.pdf)
compare-lcvsd0-vs-data.pdf
$v_2$  of Prompt $\Lambda_c^+$  and Prompt $D^0$ in Pb--Pb collisions at 5.36 TeV compared with models and light flavor from published data with $KE_T$ NCQ scaling
Energy
5.36 TeV
System
Pb-Pb
Scope: PWG
PWG-HF (Heavy Flavour)
Figure image (.eps)
compare-lcvsd0-vs-datawmodel-ket-ncq_0.eps
Figure image (.pdf)
compare-lcvsd0-vs-datawmodel-ket-ncq_0.pdf
$v_2$ of Prompt $\Lambda_c^+$  and Prompt $D^0$ in Pb--Pb collisions at 5.36 TeV compared with models and light flavor from published data with $KE_T$ NCQ scaling (logx version)
Energy
5.36 TeV
System
Pb-Pb
Scope: PWG
PWG-HF (Heavy Flavour)
Figure image (.eps)
compare-lcvsd0-vs-datawmodel-ket-ncq_logx_0.eps
Figure image (.pdf)
compare-lcvsd0-vs-datawmodel-ket-ncq_logx_0.pdf
$v_2$ of Prompt $\Lambda_c^+$  and Prompt $D^0$ in Pb--Pb collisions at 5.36 TeV compared with models and light flavor from published data with $p_T$ NCQ scaling (logx version)
Energy
5.36 TeV
System
Pb-Pb
Scope: PWG
PWG-HF (Heavy Flavour)
Figure image (.eps)
compare-lcvsd0-vs-datawmodel-pt-ncq_logx.eps
Figure image (.pdf)
compare-lcvsd0-vs-datawmodel-pt-ncq_logx.pdf
$v_2$ of Prompt $\Lambda_c^+$  and Prompt $D^0$ in Pb--Pb collisions at 5.36 TeV compared with models and light flavor from published data with $p_T$ NCQ scaling
Energy
5.36 TeV
System
Pb-Pb
Scope: PWG
PWG-HF (Heavy Flavour)
Figure image (.eps)
compare-lcvsd0-vs-datawmodel-pt-ncq_0.eps
Figure image (.pdf)
compare-lcvsd0-vs-datawmodel-pt-ncq_0.pdf
$v_2$ of Prompt $\Lambda_c^+$ and Prompt $D^0$ in Pb--Pb collisions at 5.36 TeV compared with models and light flavor from published data with $KE_T$ NCQ scaling ($KE_T$<3.3 version)
Energy
5.36 TeV
System
Pb-Pb
Scope: PWG
PWG-HF (Heavy Flavour)
Figure image (.eps)
compare-lcvsd0-vs-datawmodel-ket-ncq-ketmax3_0.eps
Figure image (.pdf)
compare-lcvsd0-vs-datawmodel-ket-ncq-ketmax3_0.pdf
Simultaneous fit of the invariant-mass distribution and $v_2$ versus invariant mass of $\Lambda_c^+$ candidates in the 4 < $p_T$< 5 GeV/c interval (0 < BDT score to be prompt < 0.03).
Energy
5.36 TeV
System
Pb-Pb
Scope: PWG
PWG-HF (Heavy Flavour)
Figure image (.eps)
lc_invmassfitpass4-pt4-5-00.eps
Figure image (.pdf)
lc_invmassfitpass4-pt4-5-00.pdf
Simultaneous fit of the invariant-mass distribution and $v_2$ versus invariant mass of $\Lambda_c^+$ candidates in the 4 < $p_T$< 5 GeV/c interval (0.03 < BDT score to be prompt < 0.8).
Energy
5.36 TeV
System
Pb-Pb
Scope: PWG
PWG-HF (Heavy Flavour)
Figure image (.eps)
lc_invmassfitpass4-pt4-5-01.eps
Figure image (.pdf)
lc_invmassfitpass4-pt4-5-01.pdf
Simultaneous fit of the invariant-mass distribution and $v_2$ versus invariant mass of $\Lambda_c^+$ candidates in the 4 < $p_T$< 5 GeV/c interval (0.8 < BDT score to be prompt < 1).
Energy
5.36 TeV
System
Pb-Pb
Scope: PWG
PWG-HF (Heavy Flavour)
Figure image (.eps)
lc_invmassfitpass4-pt4-5-02.eps
Figure image (.pdf)
lc_invmassfitpass4-pt4-5-02.pdf
Observed elliptic flow as a function of non-prompt fraction for $\Lambda_c^+$ in 4 < $p_T$ < 5 GeV/c interval.
Energy
5.36 TeV
System
Pb-Pb
Scope: PWG
PWG-HF (Heavy Flavour)
Figure image (.eps)
lc_v2ffd_fitpass4-pt4-5.eps
Figure image (.pdf)
lc_v2ffd_fitpass4-pt4-5.pdf
$\Lambda_c^+$ raw yield distribution as a function of the selection applied on the BDT output score in 4 < $p_T$ < 5 GeV/c interval.
Energy
5.36 TeV
System
Pb-Pb
Scope: PWG
PWG-HF (Heavy Flavour)
Figure image (.eps)
cutvar_canv.eps
Figure image (.pdf)
cutvar_canv.pdf