# Bulk Properties of the Medium Produced in Relativistic Heavy-Ion   Collisions from the Beam Energy Scan Program

**Authors:** STAR Collaboration: L. Adamczyk, J. K. Adkins, G. Agakishiev, M. M., Aggarwal, Z. Ahammed, N. N. Ajitanand, I. Alekseev, D. M. Anderson, R., Aoyama, A. Aparin, D. Arkhipkin, E. C. Aschenauer, M. U. Ashraf, A. Attri, G., S. Averichev, X. Bai, V. Bairathi, A. Behera, R. Bellwied, A. Bhasin, A. K., Bhati, P. Bhattarai, J. Bielcik, J. Bielcikova, L. C. Bland, I. G., Bordyuzhin, J. Bouchet, J. D. Brandenburg, A. V. Brandin, D. Brown, I., Bunzarov, J. Butterworth, H. Caines, M. Calder\'on de la Barca S\'anchez, J., M. Campbell, D. Cebra, I. Chakaberia, P. Chaloupka, Z. Chang, N., Chankova-Bunzarova, A. Chatterjee, S. Chattopadhyay, X. Chen, J. H. Chen, X., Chen, J. Cheng, M. Cherney, W. Christie, G. Contin, H. J. Crawford, S. Das,, L. C. De Silva, R. R. Debbe, T. G. Dedovich, J. Deng, A. A. Derevschikov, L., Didenko, C. Dilks, X. Dong, J. L. Drachenberg, J. E. Draper, L. E., Dunkelberger, J. C. Dunlop, L. G. Efimov, N. Elsey, J. Engelage, G. Eppley,, R. Esha, S. Esumi, O. Evdokimov, J. Ewigleben, O. Eyser, R. Fatemi, S. Fazio,, P. Federic, P. Federicova, J. Fedorisin, Z. Feng, P. Filip, E. Finch, Y., Fisyak, C. E. Flores, L. Fulek, C. A. Gagliardi, D. Garand, F. Geurts, A., Gibson, M. Girard, D. Grosnick, D. S. Gunarathne, Y. Guo, A. Gupta, S. Gupta,, W. Guryn, A. I. Hamad, A. Hamed, A. Harlenderova, J. W. Harris, L. He, S., Heppelmann, S. Heppelmann, A. Hirsch, G. W. Hoffmann, S. Horvat, T. Huang, B., Huang, X. Huang, H. Z. Huang, T. J. Humanic, P. Huo, G. Igo, W. W. Jacobs, A., Jentsch, J. Jia, K. Jiang, S. Jowzaee, E. G. Judd, S. Kabana, D. Kalinkin, K., Kang, K. Kauder, H. W. Ke, D. Keane, A. Kechechyan, Z. Khan, D. P. Kiko{\l}a,, I. Kisel, A. Kisiel, L. Kochenda, M. Kocmanek, T. Kollegger, L. K., Kosarzewski, A. F. Kraishan, P. Kravtsov, K. Krueger, N. Kulathunga, L., Kumar, J. Kvapil, J. H. Kwasizur, R. Lacey, J. M. Landgraf, K. D. Landry, J., Lauret, A. Lebedev, R. Lednicky, J. H. Lee, X. Li, C. Li, W. Li, Y. Li, J., Lidrych, T. Lin, M. A. Lisa, H. Liu, P. Liu, Y. Liu, F. Liu, T. Ljubicic, W., J. Llope, M. Lomnitz, R. S. Longacre, S. Luo, X. Luo, G. L. Ma, L. Ma, Y. G., Ma, R. Ma, N. Magdy, R. Majka, D. Mallick, S. Margetis, C. Markert, H. S., Matis, K. Meehan, J. C. Mei, Z. W. Miller, N. G. Minaev, S. Mioduszewski, D., Mishra, S. Mizuno, B. Mohanty, M. M. Mondal, D. A. Morozov, M. K. Mustafa,, Md. Nasim, T. K. Nayak, J. M. Nelson, M. Nie, G. Nigmatkulov, T. Niida, L. V., Nogach, T. Nonaka, S. B. Nurushev, G. Odyniec, A. Ogawa, K. Oh, V. A., Okorokov, D. Olvitt Jr., B. S. Page, R. Pak, Y. Pandit, Y. Panebratsev, B., Pawlik, H. Pei, C. Perkins, P. Pile, J. Pluta, K. Poniatowska, J. Porter, M., Posik, A. M. Poskanzer, N. K. Pruthi, M. Przybycien, J. Putschke, H. Qiu, A., Quintero, S. Ramachandran, R. L. Ray, R. Reed, M. J. Rehbein, H. G. Ritter,, J. B. Roberts, O. V. Rogachevskiy, J. L. Romero, J. D. Roth, L. Ruan, J., Rusnak, O. Rusnakova, N. R. Sahoo, P. K. Sahu, S. Salur, J. Sandweiss, M., Saur, J. Schambach, A. M. Schmah, W. B. Schmidke, N. Schmitz, B. R. Schweid,, J. Seger, M. Sergeeva, P. Seyboth, N. Shah, E. Shahaliev, P. V., Shanmuganathan, M. Shao, A. Sharma, M. K. Sharma, W. Q. Shen, Z. Shi, S. S., Shi, Q. Y. Shou, E. P. Sichtermann, R. Sikora, M. Simko, S. Singha, M. J., Skoby, N. Smirnov, D. Smirnov, W. Solyst, L. Song, P. Sorensen, H. M. Spinka,, B. Srivastava, T. D. S. Stanislaus, M. Strikhanov, B. Stringfellow, T., Sugiura, M. Sumbera, B. Summa, Y. Sun, X. M. Sun, X. Sun, B. Surrow, D. N., Svirida, A. H. Tang, Z. Tang, A. Taranenko, T. Tarnowsky, A. Tawfik, J., Th\"ader, J. H. Thomas, A. R. Timmins, D. Tlusty, T. Todoroki, M. Tokarev, S., Trentalange, R. E. Tribble, P. Tribedy, S. K. Tripathy, B. A. Trzeciak, O. D., Tsai, T. Ullrich, D. G. Underwood, I. Upsal, G. Van Buren, G. van, Nieuwenhuizen, A. N. Vasiliev, F. Videb{\ae}k, S. Vokal, S. A. Voloshin, A., Vossen, G. Wang, Y. Wang, F. Wang, Y. Wang, J. C. Webb, G. Webb, L. Wen, G., D. Westfall, H. Wieman, S. W. Wissink, R. Witt, Y. Wu, Z. G. Xiao, W. Xie, G., Xie, J. Xu, N. Xu, Q. H. Xu, Y. F. Xu, Z. Xu, Y. Yang, Q. Yang, C. Yang, S., Yang, Z. Ye, Z. Ye, L. Yi, K. Yip, I. -K. Yoo, N. Yu, H. Zbroszczyk, W. Zha,, Z. Zhang, X. P. Zhang, J. B. Zhang, S. Zhang, J. Zhang, Y. Zhang, J. Zhang,, S. Zhang, J. Zhao, C. Zhong, L. Zhou, C. Zhou, X. Zhu, Z. Zhu, M. Zyzak

arXiv: 1701.07065 · 2017-10-18

## TL;DR

This paper reports systematic measurements of bulk properties of matter produced in gold-gold collisions at various energies, revealing insights into the chemical and kinetic freeze-out conditions across a broad energy range at RHIC.

## Contribution

It provides new systematic data on bulk properties and freeze-out dynamics in heavy-ion collisions over a wide energy spectrum at RHIC.

## Key findings

- Particle yields and ratios vary with collision energy and centrality.
- Freeze-out parameters show energy dependence, indicating changing chemical and kinetic conditions.
- Results help map the QCD phase diagram at different baryon chemical potentials.

## Abstract

We present measurements of bulk properties of the matter produced in Au+Au collisions at $\sqrt{s_{NN}}=$ 7.7, 11.5, 19.6, 27, and 39 GeV using identified hadrons ($\pi^\pm$, $K^\pm$, $p$ and $\bar{p}$) from the STAR experiment in the Beam Energy Scan (BES) Program at the Relativistic Heavy Ion Collider (RHIC). Midrapidity ($|y|<$0.1) results for multiplicity densities $dN/dy$, average transverse momenta $\langle p_T \rangle$ and particle ratios are presented. The chemical and kinetic freeze-out dynamics at these energies are discussed and presented as a function of collision centrality and energy. These results constitute the systematic measurements of bulk properties of matter formed in heavy-ion collisions over a broad range of energy (or baryon chemical potential) at RHIC.

## Full text

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## Figures

56 figures with captions in the complete paper: https://tomesphere.com/paper/1701.07065/full.md

## References

94 references — full list in the complete paper: https://tomesphere.com/paper/1701.07065/full.md

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Source: https://tomesphere.com/paper/1701.07065