STOS(TM1) (original version)
Abstract
This table contains the EoS of H. Shen, H. Toki, K. Oyamatsu, and K. Sumiyoshi [STOSP_1998,STOSN_1998] with only baryonic contributions (no leptons or photons included) using a non-linear relativistic mean-field model with the TM1 parametrization [STNP_1994] of the effective interaction. Non-uniform nuclear matter is calculated in the single-nucleus Thomas-Fermi approximation with parametrized density distributions in spherical Wigner-Seitz cells. Only neutrons, protons, alpha particles and a single heavy nucleus are considered. The present table is the original version that was taken from the website user.numazu-ct.ac.jp/ of K. Sumiyoshi. An update with higher resolution (new version) is available in the CompOSE database.
| Nparam | = | 3 |
| Particles | = | npaNR |
| T min | = | 1.00e-01 |
| T max | = | 1.00e+02 |
| T pts | = | 31 |
| nb min | = | 7.59e-11 |
| nb max | = | 1.73e+00 |
| nb pts | = | 104 |
| Y min | = | 1.00e-02 |
| Y max | = | 5.62e-01 |
| Y pts | = | 71 |
Nuclear Matter Properties
| ns | = | 0.145 | fm-3 |
| E0 | = | 16.26 | Mev |
| K | = | 281.16 | Mev |
| K' | = | -285.22 | Mev |
| J | = | 36.89 | Mev |
| L | = | 110.79 | Mev |
| Ksym | = | 33.62 | MeV |
Neutron Star Properties
| Mmax | = | N/A | Msun |
| MDU,e | = | N/A | Msun |
| RMmax | = | N/A | km |
| R1.4 | = | N/A | km |
References
References to the original work:
- [STOSP_1998] H. Shen, H. Toki, K. Oyamatsu, K. Sumiyoshi, Prog. Theor. Phys. 100, 1013 (1998)
- [STOSN_1998] H. Shen, H. Toki, K. Oyamatsu, K. Sumiyoshi, Nucl. Phys. A 637, 435 (1998)
Further references:
- [STNP_1994] Y. Sugahara, H. Toki, Nucl. Phys. A 579, 557 (1994)
Data sheet
Data
| eos.zip (16.86 MB) |
| eos.zip_checksum.txt |
Single files |
| eos.compo |
| eos.init |
| eos.micro |
| eos.nb |
| eos.t |
| eos.thermo |
| eos.yq |