Dense Nuclear Matter Equation of State from Heavy-Ion Collisions
Agnieszka Sorensen, Kshitij Agarwal, Kyle W. Brown, Zbigniew Chajęcki, Paweł Danielewicz, Christian Drischler, Stefano Gandolfi, Jeremy W. Holt, Matthias Kamins… 展开作者
Agnieszka Sorensen, Kshitij Agarwal, Kyle W. Brown, Zbigniew Chajęcki, Paweł Danielewicz, Christian Drischler, Stefano Gandolfi, Jeremy W. Holt, Matthias Kaminski, Che-Ming Ko, Rohit Kumar, Bao-An Li, William G. Lynch, Alan B. McIntosh, William G. Newton, Scott Pratt, Oleh Savchuk, Maria Stefaniak, Ingo Tews, ManYee Betty Tsang, Ramona Vogt, Hermann Wolter, Hanna Zbroszczyk, Navid Abbasi, Jörg Aichelin, Anton Andronic, Steffen A. Bass, Francesco Becattini, David Blaschke, Marcus Bleicher, Christoph Blume, Elena Bratkovskaya, B. Alex Brown, David A. Brown, Alberto Camaiani, Giovanni Casini, Katerina Chatziioannou, Abdelouahad Chbihi, Maria Colonna, Mircea Dan Cozma, Veronica Dexheimer, Xin Dong, Travis Dore, Lipei Du, José A. Dueñas, Hannah Elfner, Wojciech Florkowski, Yuki Fujimoto, Richard J. Furnstahl, Alexandra Gade, Tetyana Galatyuk, Charles Gale, Frank Geurts, Fabiana Gramegna, Sašo Grozdanov, Kris Hagel, Steven P. Harris, Wick Haxton, Ulrich Heinz, Michal P. Heller, Or Hen, Heiko Hergert, Norbert Herrmann, Huan Zhong Huang, Xu-Guang Huang, Natsumi Ikeno, Gabriele Inghirami, Jakub Jankowski, Jiangyong Jia, José C. Jiménez, Joseph Kapusta, Behruz Kardan, Iurii Karpenko, Declan Keane, Dmitri Kharzeev, Andrej Kugler, Arnaud Le Fèvre, Dean Lee, Hong Liu, Michael A. Lisa, William J. Llope, Ivano Lombardo, Manuel Lorenz, Tommaso Marchi, Larry McLerran, Ulrich Mosel, Anton Motornenko, Berndt Müller, Paolo Napolitani, Joseph B. Natowitz, Witold Nazarewicz, Jorge Noronha, Jacquelyn Noronha-Hostler, Grażyna Odyniec, Panagiota Papakonstantinou, Zuzana Paulínyová, Jorge Piekarewicz, Robert D. Pisarski, Christopher Plumberg, Madappa Prakash, Jørgen Randrup, Claudia Ratti, Peter Rau, Sanjay Reddy, Hans-Rudolf Schmidt, Paolo Russotto, Radoslaw Ryblewski, Andreas Schäfer, Björn Schenke, Srimoyee Sen, Peter Senger, Richard Seto, Chun Shen, Bradley Sherrill, Mayank Singh, Vladimir Skokov, Michał Spaliński, Jan Steinheimer, Mikhail Stephanov, Joachim Stroth, Christian Sturm, Kai-Jia Sun, Aihong Tang, Giorgio Torrieri, Wolfgang Trautmann, Giuseppe Verde, Volodymyr Vovchenko, Ryoichi Wada, Fuqiang Wang, Gang Wang, Klaus Werner, Nu Xu, Zhangbu Xu, Ho-Ung Yee, Sherry Yennello, Yi Yin
备注：
White paper prepared for the 2023 Long Range Plan. v3: Updated version as published in Progress in Particle and Nuclear Physics. Note: the published version does not include the executive summary; in the updated arXiv version, the executive summary is included as an appendix. v4: Corrected list of authors
The nuclear equation of state (EOS) is at the center of numerous theoretical and experimental efforts in nuclear physics. With advances in microscopic theories for nuclear interactions, the availability of experiments probing nuclear matter under conditions not reached before, endeavors to develop sophisticated and reliable transport simulations to interpret these experiments, and the advent of multi-messenger astronomy, the next decade will bring new opportunities for determining the nuclear matter EOS, elucidating its dependence on density, temperature, and isospin asymmetry. Among controlled terrestrial experiments, collisions of heavy nuclei at intermediate beam energies (from a few tens of MeV/nucleon to about 25 GeV/nucleon in the fixed-target frame) probe the widest ranges of baryon density and temperature, enabling studies of nuclear matter from a few tenths to about 5 times the nuclear saturation density and for temperatures from a few to well above a hundred MeV, respectively. Collisions of neutron-rich isotopes further bring the opportunity to probe effects due to the isospin asymmetry. However, capitalizing on the enormous scientific effort aimed at uncovering the dense nuclear matter EOS, both at RHIC and at FRIB as well as at other international facilities, depends on the continued development of state-of-the-art hadronic transport simulations. This white paper highlights the essential role that heavy-ion collision experiments and hadronic transport simulations play in understanding strong interactions in dense nuclear matter, with an emphasis on how these efforts can be used together with microscopic approaches and neutron star studies to uncover the nuclear EOS.
Alpha clustering in warm and dense nuclear matter from heavy-ion collisions
Fudan University（复旦大学）；Shanghai Institute of Applied Physics, Chinese Academy of Sciences（中国科学院上海应用物理研究所）；Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Catania（意大利国家核物理研究所卡塔尼亚分部）；Sino-French Institute of Nuclear Engineering and Technology, Sun Yat-Sen University（中山大学中法核工程与技术学院）；Shanghai Research Center for Theoretical Nuclear Physics, NSFC and Fudan University（国家自然科学基金委与复旦大学理论核物理上海研究中心）；School of Physics and Astronomy, Shanghai Jiao Tong University（上海交通大学物理与天文学院）；Cyclotron Institute and Department of Physics and Astronomy, Texas A&M University（德克萨斯农工大学回旋仪研究所及物理与天文系）
Extraction of ground-state nuclear deformations from ultra-relativistic heavy-ion collisions: Nuclear structure physics context
University of York（约克大学）；University of Warsaw（华沙大学）；Michigan State University（密歇根州立大学）；University of North Carolina at Chapel Hill（北卡罗来纳大学教堂山分校）；Duke University（杜克大学）
Simulation of heavy ion collision using a time-dependent density functional theory including nuclear superfluidity
利用含时密度泛函理论对重离子碰撞进行了模拟。我们称之为正则基含时Hartree-Fock-Bogoliubov理论（Cb-TDHFB），它可以在三维坐标空间中描述核动力学，处理核对关联。我们用具有接触型配对泛函的Cb-TDHFB方法模拟了20 O +20 O碰撞，并给出了碰撞过程中带隙能量的衰减和振动行为.
Effects of momentum-dependent nuclear potential on two-nucleon correlation functions and light cluster production in intermediate energy heavy-ion collisions
