Auxiliary Function Approach for Determining Symmetry Energy at Supra-saturation Densities
| Title: | Auxiliary Function Approach for Determining Symmetry Energy at Supra-saturation Densities |
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| Authors: | Cai, Bao-Jun, Li, Bao-An |
| Source: | Phys. Rev. C 103, 054611 (2021) |
| Publication Year: | 2021 |
| Collection: | Astrophysics Nuclear Experiment Nuclear Theory |
| Subject Terms: | Nuclear Theory, Astrophysics - High Energy Astrophysical Phenomena, Nuclear Experiment |
| More Details: | Nuclear symmetry energy $E_{\rm{sym}}(\rho)$ at density $\rho$ is normally expanded or simply parameterized as a function of $\chi=(\rho-\rho_0)/3\rho_0$ in the form of $E_{\rm{sym}}(\rho)\approx S+L\chi+2^{-1}K_{\rm{sym}}\chi^2+6^{-1}J_{\rm{sym}}\chi^3+\cdots$ using its magnitude $S$, slope $L $, curvature $K_{\rm{sym}}$ and skewness $J_{\rm{sym}}$ at the saturation density $\rho_0$ of nuclear matter. Much progress has been made in recent years in constraining especially the $S$ and $L$ parameters using various terrestrial experiments and astrophysical observations. However, such kind of expansions/parameterizations do not converge at supra-saturation densities where $\chi$ is not small enough, hindering an accurate determination of high-density $E_{\rm{sym}}(\rho)$ even if its characteristic parameters at $\rho_0$ are all well determined by experiments/observations. By expanding the $E_{\rm{sym}}(\rho)$ in terms of a properly chosen auxiliary function $\Pi_{\rm{sym}}(\chi,\Theta_{\rm{sym}})$ with a parameter $\Theta_{\rm{sym}}$ fixed accurately by an experimental $E_{\rm{sym}}(\rho_{\rm{r}})$ value at a reference density $\rho_{\rm{r}}$, we show that the shortcomings of the $\chi$-expansion can be completely removed or significantly reduced in determining the high-density behavior of $E_{\rm{sym}}(\rho)$. In particular, using two significantly different auxiliary functions, we show that the new approach effectively incorporates higher $\chi$-order contributions and converges to the same $E_{\rm{sym}}(\rho)$ much faster than the conventional $\chi$-expansion at densities $\lesssim3\rho_0$. Several quantitative demonstrations using Monte Carlo simulations are given. Comment: Discussions and references added. Phys. Rev. C in press |
| Document Type: | Working Paper |
| DOI: | 10.1103/PhysRevC.103.054611 |
| Access URL: | http://arxiv.org/abs/2104.02185 |
| Accession Number: | edsarx.2104.02185 |
| Database: | arXiv |
| DOI: | 10.1103/PhysRevC.103.054611 |
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