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Dense Nuclear Matter Equation of State from Heavy-Ion Collisions

Fuente: arXiv

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Auteurs principaux:	Sorensen, Agnieszka, Agarwal, Kshitij, Brown, Kyle W., Chajęcki, Zbigniew, Danielewicz, Paweł, Drischler, Christian, Gandolfi, Stefano, Holt, Jeremy W., Kaminski, Matthias, Ko, Che-Ming, Kumar, Rohit, Li, Bao-An, Lynch, William G., McIntosh, Alan B., Newton, William G., Pratt, Scott, Savchuk, Oleh, Stefaniak, Maria, Tews, Ingo, Tsang, ManYee Betty, Vogt, Ramona, Wolter, Hermann, Zbroszczyk, Hanna, Abbasi, Navid, Aichelin, Jörg, Andronic, Anton, Bass, Steffen A., Becattini, Francesco, Blaschke, David, Bleicher, Marcus, Blume, Christoph, Bratkovskaya, Elena, Brown, B. Alex, Brown, David A., Camaiani, Alberto, Casini, Giovanni, Chatziioannou, Katerina, Chbihi, Abdelouahad, Colonna, Maria, Cozma, Mircea Dan, Dexheimer, Veronica, Dong, Xin, Dore, Travis, Du, Lipei, Dueñas, José A., Elfner, Hannah, Florkowski, Wojciech, Fujimoto, Yuki, Furnstahl, Richard J., Gade, Alexandra, Galatyuk, Tetyana, Gale, Charles, Geurts, Frank, Gramegna, Fabiana, Grozdanov, Sašo, Hagel, Kris, Harris, Steven P., Haxton, Wick, Heinz, Ulrich, Heller, Michal P., Hen, Or, Hergert, Heiko, Herrmann, Norbert, Huang, Huan Zhong, Huang, Xu-Guang, Ikeno, Natsumi, Inghirami, Gabriele, Jankowski, Jakub, Jia, Jiangyong, Jiménez, José C., Kapusta, Joseph, Kardan, Behruz, Karpenko, Iurii, Keane, Declan, Kharzeev, Dmitri, Kugler, Andrej, Fèvre, Arnaud Le, Lee, Dean, Liu, Hong, Lisa, Michael A., Llope, William J., Lombardo, Ivano, Lorenz, Manuel, Marchi, Tommaso, McLerran, Larry, Mosel, Ulrich, Motornenko, Anton, Müller, Berndt, Napolitani, Paolo, Natowitz, Joseph B., Nazarewicz, Witold, Noronha, Jorge, Noronha-Hostler, Jacquelyn, Odyniec, Grażyna, Papakonstantinou, Panagiota, Paulínyová, Zuzana, Piekarewicz, Jorge, Pisarski, Robert D., Plumberg, Christopher, Prakash, Madappa, Randrup, Jørgen, Ratti, Claudia, Rau, Peter, Reddy, Sanjay, Schmidt, Hans-Rudolf, Russotto, Paolo, Ryblewski, Radoslaw, Schäfer, Andreas, Schenke, Björn, Sen, Srimoyee, Senger, Peter, Seto, Richard, Shen, Chun, Sherrill, Bradley, Singh, Mayank, Skokov, Vladimir, Spaliński, Michał, Steinheimer, Jan, Stephanov, Mikhail, Stroth, Joachim, Sturm, Christian, Sun, Kai-Jia, Tang, Aihong, Torrieri, Giorgio, Trautmann, Wolfgang, Verde, Giuseppe, Vovchenko, Volodymyr, Wada, Ryoichi, Wang, Fuqiang, Wang, Gang, Werner, Klaus, Xu, Nu, Xu, Zhangbu, Yee, Ho-Ung, Yennello, Sherry, Yin, Yi
Format:	Preprint
Publié:	2023
Sujets:	Nuclear Theory Nuclear Experiment
Accès en ligne:	Acceder al recurso
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_version_	1866913209667026944
author	Sorensen, Agnieszka Agarwal, Kshitij Brown, Kyle W. Chajęcki, Zbigniew Danielewicz, Paweł Drischler, Christian Gandolfi, Stefano Holt, Jeremy W. Kaminski, Matthias Ko, Che-Ming Kumar, Rohit Li, Bao-An Lynch, William G. McIntosh, Alan B. Newton, William G. Pratt, Scott Savchuk, Oleh Stefaniak, Maria Tews, Ingo Tsang, ManYee Betty Vogt, Ramona Wolter, Hermann Zbroszczyk, Hanna Abbasi, Navid Aichelin, Jörg Andronic, Anton Bass, Steffen A. Becattini, Francesco Blaschke, David Bleicher, Marcus Blume, Christoph Bratkovskaya, Elena Brown, B. Alex Brown, David A. Camaiani, Alberto Casini, Giovanni Chatziioannou, Katerina Chbihi, Abdelouahad Colonna, Maria Cozma, Mircea Dan Dexheimer, Veronica Dong, Xin Dore, Travis Du, Lipei Dueñas, José A. Elfner, Hannah Florkowski, Wojciech Fujimoto, Yuki Furnstahl, Richard J. Gade, Alexandra Galatyuk, Tetyana Gale, Charles Geurts, Frank Gramegna, Fabiana Grozdanov, Sašo Hagel, Kris Harris, Steven P. Haxton, Wick Heinz, Ulrich Heller, Michal P. Hen, Or Hergert, Heiko Herrmann, Norbert Huang, Huan Zhong Huang, Xu-Guang Ikeno, Natsumi Inghirami, Gabriele Jankowski, Jakub Jia, Jiangyong Jiménez, José C. Kapusta, Joseph Kardan, Behruz Karpenko, Iurii Keane, Declan Kharzeev, Dmitri Kugler, Andrej Fèvre, Arnaud Le Lee, Dean Liu, Hong Lisa, Michael A. Llope, William J. Lombardo, Ivano Lorenz, Manuel Marchi, Tommaso McLerran, Larry Mosel, Ulrich Motornenko, Anton Müller, Berndt Napolitani, Paolo Natowitz, Joseph B. Nazarewicz, Witold Noronha, Jorge Noronha-Hostler, Jacquelyn Odyniec, Grażyna Papakonstantinou, Panagiota Paulínyová, Zuzana Piekarewicz, Jorge Pisarski, Robert D. Plumberg, Christopher Prakash, Madappa Randrup, Jørgen Ratti, Claudia Rau, Peter Reddy, Sanjay Schmidt, Hans-Rudolf Russotto, Paolo Ryblewski, Radoslaw Schäfer, Andreas Schenke, Björn Sen, Srimoyee Senger, Peter Seto, Richard Shen, Chun Sherrill, Bradley Singh, Mayank Skokov, Vladimir Spaliński, Michał Steinheimer, Jan Stephanov, Mikhail Stroth, Joachim Sturm, Christian Sun, Kai-Jia Tang, Aihong Torrieri, Giorgio Trautmann, Wolfgang Verde, Giuseppe Vovchenko, Volodymyr Wada, Ryoichi Wang, Fuqiang Wang, Gang Werner, Klaus Xu, Nu Xu, Zhangbu Yee, Ho-Ung Yennello, Sherry Yin, Yi
author_facet	Sorensen, Agnieszka Agarwal, Kshitij Brown, Kyle W. Chajęcki, Zbigniew Danielewicz, Paweł Drischler, Christian Gandolfi, Stefano Holt, Jeremy W. Kaminski, Matthias Ko, Che-Ming Kumar, Rohit Li, Bao-An Lynch, William G. McIntosh, Alan B. Newton, William G. Pratt, Scott Savchuk, Oleh Stefaniak, Maria Tews, Ingo Tsang, ManYee Betty Vogt, Ramona Wolter, Hermann Zbroszczyk, Hanna Abbasi, Navid Aichelin, Jörg Andronic, Anton Bass, Steffen A. Becattini, Francesco Blaschke, David Bleicher, Marcus Blume, Christoph Bratkovskaya, Elena Brown, B. Alex Brown, David A. Camaiani, Alberto Casini, Giovanni Chatziioannou, Katerina Chbihi, Abdelouahad Colonna, Maria Cozma, Mircea Dan Dexheimer, Veronica Dong, Xin Dore, Travis Du, Lipei Dueñas, José A. Elfner, Hannah Florkowski, Wojciech Fujimoto, Yuki Furnstahl, Richard J. Gade, Alexandra Galatyuk, Tetyana Gale, Charles Geurts, Frank Gramegna, Fabiana Grozdanov, Sašo Hagel, Kris Harris, Steven P. Haxton, Wick Heinz, Ulrich Heller, Michal P. Hen, Or Hergert, Heiko Herrmann, Norbert Huang, Huan Zhong Huang, Xu-Guang Ikeno, Natsumi Inghirami, Gabriele Jankowski, Jakub Jia, Jiangyong Jiménez, José C. Kapusta, Joseph Kardan, Behruz Karpenko, Iurii Keane, Declan Kharzeev, Dmitri Kugler, Andrej Fèvre, Arnaud Le Lee, Dean Liu, Hong Lisa, Michael A. Llope, William J. Lombardo, Ivano Lorenz, Manuel Marchi, Tommaso McLerran, Larry Mosel, Ulrich Motornenko, Anton Müller, Berndt Napolitani, Paolo Natowitz, Joseph B. Nazarewicz, Witold Noronha, Jorge Noronha-Hostler, Jacquelyn Odyniec, Grażyna Papakonstantinou, Panagiota Paulínyová, Zuzana Piekarewicz, Jorge Pisarski, Robert D. Plumberg, Christopher Prakash, Madappa Randrup, Jørgen Ratti, Claudia Rau, Peter Reddy, Sanjay Schmidt, Hans-Rudolf Russotto, Paolo Ryblewski, Radoslaw Schäfer, Andreas Schenke, Björn Sen, Srimoyee Senger, Peter Seto, Richard Shen, Chun Sherrill, Bradley Singh, Mayank Skokov, Vladimir Spaliński, Michał Steinheimer, Jan Stephanov, Mikhail Stroth, Joachim Sturm, Christian Sun, Kai-Jia Tang, Aihong Torrieri, Giorgio Trautmann, Wolfgang Verde, Giuseppe Vovchenko, Volodymyr Wada, Ryoichi Wang, Fuqiang Wang, Gang Werner, Klaus Xu, Nu Xu, Zhangbu Yee, Ho-Ung Yennello, Sherry Yin, Yi
contents	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.
format	Preprint
id	arxiv_https___arxiv_org_abs_2301_13253
institution	arXiv
publishDate	2023
record_format	arxiv
spellingShingle	Dense Nuclear Matter Equation of State from Heavy-Ion Collisions Sorensen, Agnieszka Agarwal, Kshitij Brown, Kyle W. Chajęcki, Zbigniew Danielewicz, Paweł Drischler, Christian Gandolfi, Stefano Holt, Jeremy W. Kaminski, Matthias Ko, Che-Ming Kumar, Rohit Li, Bao-An Lynch, William G. McIntosh, Alan B. Newton, William G. Pratt, Scott Savchuk, Oleh Stefaniak, Maria Tews, Ingo Tsang, ManYee Betty Vogt, Ramona Wolter, Hermann Zbroszczyk, Hanna Abbasi, Navid Aichelin, Jörg Andronic, Anton Bass, Steffen A. Becattini, Francesco Blaschke, David Bleicher, Marcus Blume, Christoph Bratkovskaya, Elena Brown, B. Alex Brown, David A. Camaiani, Alberto Casini, Giovanni Chatziioannou, Katerina Chbihi, Abdelouahad Colonna, Maria Cozma, Mircea Dan Dexheimer, Veronica Dong, Xin Dore, Travis Du, Lipei Dueñas, José A. Elfner, Hannah Florkowski, Wojciech Fujimoto, Yuki Furnstahl, Richard J. Gade, Alexandra Galatyuk, Tetyana Gale, Charles Geurts, Frank Gramegna, Fabiana Grozdanov, Sašo Hagel, Kris Harris, Steven P. Haxton, Wick Heinz, Ulrich Heller, Michal P. Hen, Or Hergert, Heiko Herrmann, Norbert Huang, Huan Zhong Huang, Xu-Guang Ikeno, Natsumi Inghirami, Gabriele Jankowski, Jakub Jia, Jiangyong Jiménez, José C. Kapusta, Joseph Kardan, Behruz Karpenko, Iurii Keane, Declan Kharzeev, Dmitri Kugler, Andrej Fèvre, Arnaud Le Lee, Dean Liu, Hong Lisa, Michael A. Llope, William J. Lombardo, Ivano Lorenz, Manuel Marchi, Tommaso McLerran, Larry Mosel, Ulrich Motornenko, Anton Müller, Berndt Napolitani, Paolo Natowitz, Joseph B. Nazarewicz, Witold Noronha, Jorge Noronha-Hostler, Jacquelyn Odyniec, Grażyna Papakonstantinou, Panagiota Paulínyová, Zuzana Piekarewicz, Jorge Pisarski, Robert D. Plumberg, Christopher Prakash, Madappa Randrup, Jørgen Ratti, Claudia Rau, Peter Reddy, Sanjay Schmidt, Hans-Rudolf Russotto, Paolo Ryblewski, Radoslaw Schäfer, Andreas Schenke, Björn Sen, Srimoyee Senger, Peter Seto, Richard Shen, Chun Sherrill, Bradley Singh, Mayank Skokov, Vladimir Spaliński, Michał Steinheimer, Jan Stephanov, Mikhail Stroth, Joachim Sturm, Christian Sun, Kai-Jia Tang, Aihong Torrieri, Giorgio Trautmann, Wolfgang Verde, Giuseppe Vovchenko, Volodymyr Wada, Ryoichi Wang, Fuqiang Wang, Gang Werner, Klaus Xu, Nu Xu, Zhangbu Yee, Ho-Ung Yennello, Sherry Yin, Yi Nuclear Theory Nuclear Experiment 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.
title	Dense Nuclear Matter Equation of State from Heavy-Ion Collisions
topic	Nuclear Theory Nuclear Experiment
url	https://arxiv.org/abs/2301.13253