27 September 2015 to 3 October 2015
Kobe, Fashion Mart, Japan
Japan timezone

$\Lambda_\mathrm{c}^+$ baryon production in Au+Au collisions at $\sqrt{s_{\mathrm{NN}}}$ = 200 GeV

29 Sept 2015, 16:30
2h
Exhibition space 3 & 4

Exhibition space 3 & 4

Board: 0555
Poster Open Heavy Flavors and Strangeness Poster Session

Speaker

Miroslav Simko (Nuclear Physics Institute of the CAS (CZ))

Description

Baryon/meson ratios (p/$\pi$, $\Lambda$/K$^0_\mathrm{s}$) are observed to be significantly enhanced in central heavy-ion collisions compared with peripheral heavy-ion collisions and p+p collisions at RHIC and LHC. Several model calculations suggest that coalescence hadronization between charm quarks and light quarks will also lead to an enhancement in the $\Lambda_\mathrm{c}$/D$^0$ ratio. Therefore, it is of great interest to study the $\Lambda_\mathrm{c}$ baryon production to further understand the hadronization scheme in the charm sector and constrain total charm yield in heavy-ion collisions. The possible $\Lambda_\mathrm{c}$/D$^0$ enhancement in heavy-ion collisions will introduce additional suppression for charm decay electrons due to smaller semi-leptonic decay branching ratios of $\Lambda_\mathrm{c}$, which could lead to a different interpretation of the heavy flavor decay electron results. $\Lambda_\mathrm{c}$ baryons have an extremely small lifetime ($c \tau \sim 60$ $\mu$m) and have not been measured in heavy-ion collisions yet. The newly installed STAR Heavy Flavor Tracker (HFT) has shown high efficiency and a superior pointing resolution that facilitate the reconstruction of hadronic decays in heavy-ion collisions. In 2014 run, STAR has collected 1.2 B events of minimum bias Au+Au collisions $\sqrt{s_\mathrm{NN}}$ = 200 GeV. In this poster, we will discuss the feasibility of $\Lambda_\mathrm{c}$ measurement with the HFT in Au+Au collisions. We will report reconstruction of $\Lambda_\mathrm{c}$ baryons via hadronic decays, including decay channels through the involvement of various intermediate resonance states using 2014 Au+Au data at $\sqrt{s_\mathrm{NN}}$ = 200 GeV. In addition, we will discuss the improvement on $\Lambda_\mathrm{c}$ reconstruction using the HFT with reduced material that is taking data in 2015 (p+p, p+A) and is planned for future 2016 (Au+Au) collisions.
On behalf of collaboration: STAR

Primary author

Miroslav Simko (Nuclear Physics Institute of the CAS (CZ))

Presentation materials