Equation of state (EOS) based on the variational many-body theory with realistic nuclear forces is provided. For uniform matter, the EOS is constructed with the cluster variational method starting from the Argonne v18 two-body nuclear potential and the Urbana IX three-body nuclear potential. Non-uniform nuclear matter is treated in the Thomas-Fermi approximation. Alpha particle mixing is also taken into account. See Togashi et al., Nucl. Phys. A 961 (2017) 78 for details. This EOS table is open for general use in any studies for nuclear physics and astrophysics, provided that our paper is referred to in your publication.
User's Guide (read me first)
- Hajime Togashi
Nishina Center for Accelerator-Based Science, RIKEN
2-1 Hirosawa, Wako, Saitama 351-0198, Japan
Please refer to the following paper when you publish scientific articles using this EOS.
Nuclear equation of state for core-collapse supernova simulations with realistic nuclear forces
H. Togashi, K. Nakazato, Y. Takehara, S. Yamamuro, H. Suzuki and M. Takano,
Nucl. Phys. A 961 (2017) 78, arXiv:1702.05324 [nucl-th]
Last update, March 08, 2017