Paper proposal of PID v2 at colliding energy 7.7 - 19.6 GeV

 

Paper Title: Probing the QCD phase structure with elliptic flow in Au + Au collisions at $\sqrt{s_{NN}}$ = 7.7 - 19.6 GeV at RHIC


Target journal:
Phys. Rev. Lett.

PAs:
Prabhupada Dixit, Xin Dong, Li-Ke Liu, Md. Nasim, Sooraj Radhakrishnan, Priyanshi Sinha, Shusu Shi, Guoping Wang, Xing Wu, Nu Xu, Shuai Zhou 

PA representative
: Xing Wu
-----------------------------------------------------------------------------------------------------------------------------------------------------------------
-----------------------------------------------------------------------------------------------------------------------------------------------------------------
Abstract:

Elliptic flow ($v_2$) is sensitive to the dynamics of heavy-ion collisions at the early stage of system evolution and the degrees of freedom of the medium. With the enhanced statistical datasets from the second phase of RHIC Beam Energy Scan (BES-II) program at STAR, measurements of $v_2$ for ${\pi}^{\pm}$, ${K}^{\pm}$, ${K}^{0}_{s}$, $p$, $\bar{p}$, ${\phi}$, ${\Lambda}$, $\bar{\Lambda}$, ${\Xi}^{\pm}$ and ${\Omega}^{\pm}$ at $\sqrt{s_{NN}}$ = 7.7 - 19.6 GeV are presented. Number of Constituent Quark (NCQ) scaling is tested separately for particles and anti-particles. The NCQ scaled $v_2$ ratios of ${\pi}^{+}$/${K}^{+}$, $p$/${K}^{+}$, ${\pi}^{-}$/${K}^{-}$, $\bar{p}$/${K}^{-}$, ${\phi}$/${K}^{-}$, ${\Lambda}$/${K}^{0}_{s}$, $\bar{\Lambda}$/${K}^{0}_{s}$ are found to be close to 1 and less sensitive to the collision energy within the range of $\sqrt{s_{NN}}$ = 7.7 - 19.6 GeV. These measurements indicate that the system is dominated by partonic degrees of freedom in Au+Au collisions at $\sqrt{s_{NN}}$ = 7.7 - 19.6 GeV.

-----------------------------------------------------------------------------------------------------------------------------------------------------------------
-----------------------------------------------------------------------------------------------------------------------------------------------------------------
Paper figures:
Fig.1.: Invariant mass distribution of $\phi$, $K^{0}_{S}$, $\Lambda$, $\bar{\Lambda}$, $\Xi^{\pm}$ and $\Omega^{\pm}$ at {\rootsNN} = 14.6 GeV.
Fig.2.: The NCQ-scaled elliptic flow, $v_2$/$n_q$ VS. ($m_T - m_0$)/$n_q$ for 10-40\% centrality in Au + Au collisions is shown for particles, along with the NCQ scaling ratios to the $K_S^0$ fitting function. The dash line represents the K$E_T/$$n_q$ range from 0.3 to 1.3. The bars and brackets represent the statistical and systematic errors respectively.
Fig.3.: The NCQ-scaled elliptic flow, $v_2$/$n_q$ VS. ($m_T - m_0$)/$n_q$ for 10-40\% centrality in Au + Au collisions is shown for anti-particles, along with the NCQ scaling ratios to the $K_S^0$ fitting function. The dash line represents the K$E_T/$$n_q$ range from 0.3 to 1.3. The bars and brackets represent the statistical and systematic errors respectively.

Fig.4.: (a): The energy dependence of NCQ-scaled $v_2$ ratios for $\pi^+$/$K^+$, $p$/$K^+$ and $\Lambda$/$K_S^0$ at K$E_T$/$n_q$ = 0.4 GeV/$c^2$ in 10-40\% centrality in Au + Au collisions at $\sqrt{s_{NN}}$ = 3.2 - 19.6 GeV. (b): The energy dependence of NCQ-scaled $v_2$ ratios for $\pi^-$/$K^-$, $\bar{p}$/$K^-$, $\phi$/$K^-$ and $\bar{\Lambda}$/$K_S^0$ at K$E_T$/$n_q$ = 0.4 GeV/$c^2$ in 10-40\% centrality in Au + Au collisions at $\sqrt{s_{NN}}$ = 7.7 - 19.6 GeV.
-----------------------------------------------------------------------------------------------------------------------------------------------------------------
-----------------------------------------------------------------------------------------------------------------------------------------------------------------

Conclusions:

In summary, we present the elliptic flow of identified hadrons ${\pi}^{\pm}$, ${K}^{\pm}$, ${K}^{0}_{s}$, $p$, $\bar{p}$, ${\phi}$, ${\Lambda}$, $\bar{\Lambda}$, ${\Xi}^{\pm}$ and ${\Omega}^{\pm}$ at $\sqrt{s_{NN}}$ = 7.7 - 19.6 GeV from STAR BES-II. The ${\phi}$ meson $v_2$/$n_q$ does not deviate from other particles and anti-particles.And the NCQ scaled $v_2$ ratios of ${\pi}^{+}$/${K}^{+}$, $p$/${K}^{+}$, ${\pi}^{-}$/${K}^{-}$, $\bar{p}$/${K}^{-}$, ${\phi}$/${K}^{-}$, ${\Lambda}$/${K}^{0}_{s}$, $\bar{\Lambda}$/${K}^{0}_{s}$ are found to be close to 1 and less sensitive to the collision energy within the range of $\sqrt{s_{NN}}$ = 7.7 - 19.6 GeV. These measurements indicate that the system is dominated by partonic degrees of freedom in Au+Au collisions at $\sqrt{s_{NN}}$ = 7.7 - 19.6 GeV.

-----------------------------------------------------------------------------------------------------------------------------------------------------------------
-----------------------------------------------------------------------------------------------------------------------------------------------------------------

Presentations:

7.7 GeV:

https://drupal.star.bnl.gov/STAR/system/files/v2_of_%28multi-%29strange_hadron_7.7_official.pdf
https://drupal.star.bnl.gov/STAR/system/files/The%20elliptic%20flow%20of%20strange%20hadrons%20and%20multistrange%20hadrons%20at%20%207.7%20GeV.pdf
https://drupal.star.bnl.gov/STAR/system/files/7.7%20GeV%20process.pdf
https://drupal.star.bnl.gov/STAR/system/files/7p7piK%20412PWG.pdf
https://drupal.star.bnl.gov/STAR/system/files/7p7pikp_v2_off_PWG.pdf

9.2 GeV:

https://drupal.star.bnl.gov/STAR/system/files/v2_of_%28multi-%29strange_hadrons_9p2_GeV.pdf

11.5 GeV:

https://drupal.star.bnl.gov/STAR/system/files/Strange_v2_11p5GeV_FCVPWG_Like.pdf

14.6 GeV:

https://drupal.star.bnl.gov/STAR/system/files/14p5_v2_Collaboration_meeting_0.pdf
https://drupal.star.bnl.gov/STAR/system/files/Elliptic%20flow%20%20of%20identified%20particles%20in%20Au%2BAu%20collisions%20at%207.7%20%2019.6%20GeV_star_collaborationzs_update_0.pdf

17.3 GeV:

https://drupal.star.bnl.gov/STAR/blog/xwu2/9p211p517p3v2PWGmeeting
https://drupal.star.bnl.gov/STAR/system/files/v2%28pt%29_of_strange_hadrons_at_9p9_11p5_17p3.pdf

19.6 GeV:

https://drupal.star.bnl.gov/STAR/system/files/Preliminary_request_19p6GeV_LikeLiu_2022_0315.pdf           
https://drupal.star.bnl.gov/STAR/blog/lliu/updatepiKpphiLambdav2FCV
https://drupal.star.bnl.gov/STAR/blog/lliu/K0sXiOmegav219p6FCV

Pervious paper proposal:

https://drupal.star.bnl.gov/STAR/system/files/Colliding_energy_paper_proposal_20240820.pdf
https://drupal.star.bnl.gov/STAR/system/files/XingWu_star_collaboration.pdf
https://drupal.star.bnl.gov/STAR/system/files/Colliding_energy_v2_preliminary.pdf