# First observation of the directed flow of $D^{0}$ and $\overline{D^0}$   in Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 200~GeV

**Authors:** STAR Collaboration: J. Adam, L. Adamczyk, J. R. Adams, J. K. Adkins,, G. Agakishiev, M. M. Aggarwal, Z. Ahammed, I. Alekseev, D. M. Anderson, R., Aoyama, A. Aparin, D. Arkhipkin, E. C. Aschenauer, M. U. Ashraf, F. Atetalla,, A. Attri, G. S. Averichev, V. Bairathi, K. Barish, A. J. Bassill, A. Behera,, R. Bellwied, A. Bhasin, A. K. Bhati, J. Bielcik, J. Bielcikova, L. C. Bland,, I. G. Bordyuzhin, J. D. Brandenburg, A. V. Brandin, J. Bryslawskyj, I., Bunzarov, J. Butterworth, H. Caines, M. Calder\'on~de~la~Barca~S\'anchez, D., Cebra, I. Chakaberia, P. Chaloupka, B. K. Chan, F-H. Chang, Z. Chang, N., Chankova-Bunzarova, A. Chatterjee, S. Chattopadhyay, J. H. Chen, X. Chen, J., Cheng, M. Cherney, W. Christie, H. J. Crawford, M. Csan\'ad, S. Das, T. G., Dedovich, I. M. Deppner, A. A. Derevschikov, L. Didenko, C. Dilks, X. Dong,, J. L. Drachenberg, J. C. Dunlop, T. Edmonds, N. Elsey, J. Engelage, G., Eppley, R. Esha, S. Esumi, O. Evdokimov, J. Ewigleben, O. Eyser, R. Fatemi,, S. Fazio, P. Federic, J. Fedorisin, Y. Feng, P. Filip, E. Finch, Y. Fisyak,, L. Fulek, C. A. Gagliardi, T. Galatyuk, F. Geurts, A. Gibson, K. Gopal, D., Grosnick, A. Gupta, W. Guryn, A. I. Hamad, A. Hamed, J. W. Harris, L. He, S., Heppelmann, S. Heppelmann, N. Herrmann, L. Holub, Y. Hong, S. Horvat, B., Huang, H. Z. Huang, S. L. Huang, T. Huang, X. Huang, T. J. Humanic, P. Huo,, G. Igo, W. W. Jacobs, C. Jena, A. Jentsch, Y. JI, J. Jia, K. Jiang, S., Jowzaee, X. Ju, E. G. Judd, S. Kabana, S. Kagamaster, D. Kalinkin, K. Kang,, D. Kapukchyan, K. Kauder, H. W. Ke, D. Keane, A. Kechechyan, M. Kelsey, Y. V., Khyzhniak, D. P. Kiko{\l}a, C. Kim, T. A. Kinghorn, I. Kisel, A. Kisiel, M., Kocan, L. Kochenda, L. K. Kosarzewski, L. Kramarik, P. Kravtsov, K. Krueger,, N. Kulathunga Mudiyanselage, L. Kumar, R. Kunnawalkam Elayavalli, J. H., Kwasizur, R. Lacey, J. M. Landgraf, J. Lauret, A. Lebedev, R. Lednicky, J. H., Lee, C. Li, W. Li, W. Li, X. Li, Y. Li, Y. Liang, R. Licenik, T. Lin, A., Lipiec, M. A. Lisa, F. Liu, H. Liu, P. Liu, P. Liu, T. Liu, X. Liu, Y. Liu,, Z. Liu, T. Ljubicic, W. J. Llope, M. Lomnitz, R. S. Longacre, S. Luo, X. Luo,, G. L. Ma, L. Ma, R. Ma, Y. G. Ma, N. Magdy, R. Majka, D. Mallick, S., Margetis, C. Markert, H. S. Matis, O. Matonoha, J. A. Mazer, K. Meehan, J. C., Mei, N. G. Minaev, S. Mioduszewski, D. Mishra, B. Mohanty, M. M. Mondal, I., Mooney, Z. Moravcova, D. A. Morozov, Md. Nasim, K. Nayak, J. M. Nelson, D. B., Nemes, M. Nie, G. Nigmatkulov, T. Niida, L. V. Nogach, T. Nonaka, G. Odyniec,, A. Ogawa, K. Oh, S. Oh, V. A. Okorokov, B. S. Page, R. Pak, Y. Panebratsev,, B. Pawlik, D. Pawlowska, H. Pei, C. Perkins, R. L. Pint\'er, J. Pluta, J., Porter, M. Posik, N. K. Pruthi, M. Przybycien, J. Putschke, A. Quintero, S., K. Radhakrishnan, S. Ramachandran, R. L. Ray, R. Reed, H. G. Ritter, J. B., Roberts, O. V. Rogachevskiy, J. L. Romero, L. Ruan, J. Rusnak, O. Rusnakova,, N. R. Sahoo, P. K. Sahu, S. Salur, J. Sandweiss, J. Schambach, W. B., Schmidke, N. Schmitz, B. R. Schweid, F. Seck, J. Seger, M. Sergeeva, R. Seto,, P. Seyboth, N. Shah, E. Shahaliev, P. V. Shanmuganathan, M. Shao, F. Shen, W., Q. Shen, S. S. Shi, Q. Y. Shou, E. P. Sichtermann, S. Siejka, R. Sikora, M., Simko, J. Singh, S. Singha, D. Smirnov, N. Smirnov, W. Solyst, P. Sorensen,, H. M. Spinka, B. Srivastava, T. D. S. Stanislaus, M. Stefaniak, D. J., Stewart, M. Strikhanov, B. Stringfellow, A. A. P. Suaide, T. Sugiura, M., Sumbera, B. Summa, X. M. Sun, Y. Sun, Y. Sun, B. Surrow, D. N. Svirida, P., Szymanski, A. H. Tang, Z. Tang, A. Taranenko, T. Tarnowsky, J. H. Thomas, A., R. Timmins, D. Tlusty, T. Todoroki, M. Tokarev, C. A. Tomkiel, S., Trentalange, R. E. Tribble, P. Tribedy, S. K. Tripathy, O. D. Tsai, B. Tu, T., Ullrich, D. G. Underwood, I. Upsal, G. Van Buren, J. Vanek, A. N. Vasiliev,, I. Vassiliev, F. Videb{\ae}k, S. Vokal, S. A. Voloshin, F. Wang, G. Wang, P., Wang, Y. Wang, Y. Wang, J. C. Webb, L. Wen, G. D. Westfall, H. Wieman, S. W., Wissink, R. Witt, Y. Wu, Z. G. Xiao, G. Xie, W. Xie, H. Xu, N. Xu, Q. H. Xu,, Y. F. Xu, Z. Xu, C. Yang, Q. Yang, S. Yang, Y. Yang, Z. Yang, Z. Ye, Z. Ye,, L. Yi, K. Yip, I. -K. Yoo, H. Zbroszczyk, W. Zha, D. Zhang, L. Zhang, S., Zhang, S. Zhang, X. P. Zhang, Y. Zhang, Z. Zhang, J. Zhao, C. Zhong, C. Zhou,, X. Zhu, Z. Zhu, M. Zurek, M. Zyzak

arXiv: 1905.02052 · 2019-10-23

## TL;DR

This paper reports the first measurement of the directed flow ($v_1$) for $D^{0}$ and $ar{D}^{0}$ mesons in Au+Au collisions at 200 GeV, revealing a significant $v_1$ slope that provides insights into the initial tilt of the quark-gluon plasma.

## Contribution

It presents the first observation of $D^{0}$ and $ar{D}^{0}$ meson directed flow in heavy-ion collisions, offering new constraints on the initial conditions and transport properties of the quark-gluon plasma.

## Key findings

- $D^{0}$ meson $dv_1/dy$ is about 25 times larger than charged kaons.
- The measured $dv_1/dy$ slope is -0.080 with statistical and systematic uncertainties.
- The results provide insights into the initial tilt and transport properties of the hot QCD medium.

## Abstract

We report the first measurement of rapidity-odd directed flow ($v_{1}$) for $D^{0}$ and $\overline{D^{0}}$ mesons at mid-rapidity ($|y| < 0.8$) in Au+Au collisions at $\sqrt{s_{\rm NN}}$ = 200\,GeV using the STAR detector at the Relativistic Heavy Ion Collider. In 10--80\% Au+Au collisions, the slope of the $v_{1}$ rapidity dependence ($dv_{1}/dy$), averaged over $D^{0}$ and $\overline{D^{0}}$ mesons, is -0.080 $\pm$ 0.017 (stat.) $\pm$ 0.016 (syst.) for transverse momentum $p_{\rm T}$ above 1.5~GeV/$c$. The absolute value of $D^0$-meson $dv_1/dy$ is about 25 times larger than that for charged kaons, with 3.4$\sigma$ significance. These data give a unique insight into the initial tilt of the produced matter, and offer constraints on the geometric and transport parameters of the hot QCD medium created in relativistic heavy-ion collisions.

## Full text

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## Figures

3 figures with captions in the complete paper: https://tomesphere.com/paper/1905.02052/full.md

## References

47 references — full list in the complete paper: https://tomesphere.com/paper/1905.02052/full.md

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Source: https://tomesphere.com/paper/1905.02052