Physics:Symmetry energy
From HandWiki
In nuclear physics, the symmetry energy reflects the variation of the binding energy of the nucleons in the nuclear matter depending on its neutron to proton ratio as a function of baryon density. Symmetry energy is an important parameter in the equation of state describing the nuclear structure of heavy nuclei and neutron stars.[1][2][3][4]
References
- ↑ Baldo, M.; Burgio, G. F. (November 2016). "The nuclear symmetry energy". Progress in Particle and Nuclear Physics 91: 203–258. doi:10.1016/j.ppnp.2016.06.006. Bibcode: 2016PrPNP..91..203B.
- ↑ Tsang, M. B.; Zhang, Y.; Danielewicz, P.; Famiano, M.; Li, Z.; Lynch, W. G.; Steiner, A. W. (2009). "Constraints on the Density Dependence of the Symmetry Energy". Physical Review Letters 102 (12): 122701. doi:10.1103/PhysRevLett.102.122701. PMID 19392271. Bibcode: 2009PhRvL.102l2701T.
- ↑ Tsang, M. B. et al. (September 2010). "Constraints on the Density Dependence of the Symmetry Energy" (in en). International Journal of Modern Physics E 19 (8n09): 1631–1638. doi:10.1142/S0218301310016041. ISSN 0218-3013. Bibcode: 2010IJMPE..19.1631T.
- ↑ Lattimer, J. M. (January 2023). "Constraints on Nuclear Symmetry Energy Parameters". Particles 6 (12): 30–56. doi:10.3390/particles6010003. Bibcode: 2023Parti...6...30L.
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