2013
DOI: 10.1103/physrevc.88.044912
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Toward a model-independent constraint of the high-density dependence of the symmetry energy

Abstract: Neutron-proton elliptic flow difference and ratio have been shown to be promising observables in the attempt to constrain the density dependence of the symmetry energy above the saturation point from heavy-ion collision data. Their dependence on model parameters like microscopic nucleon-nucleon cross-sections, compressibility of nuclear matter, optical potential, and symmetry energy parametrization is thoroughly studied. By using a parametrization of the symmetry energy derived from the momentum dependent Gogn… Show more

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Cited by 103 publications
(151 citation statements)
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References 51 publications
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“…Actually there is a variety of neutron star properties which are sensitive to SE, that is the maximum mass value and the corresponding radius, the onset of the direct Urca process, the crust-core transition density and pressure e.t.c. [2,9] Recently, there is an extended theoretical [10,11,12,13,14,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,30,31,32,33,34,57,36,37,38,39,40,41,42,43,44,45,46,47,48,49,50,51,52,53,54,55,56,…”
Section: Introductionmentioning
confidence: 99%
“…Actually there is a variety of neutron star properties which are sensitive to SE, that is the maximum mass value and the corresponding radius, the onset of the direct Urca process, the crust-core transition density and pressure e.t.c. [2,9] Recently, there is an extended theoretical [10,11,12,13,14,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,30,31,32,33,34,57,36,37,38,39,40,41,42,43,44,45,46,47,48,49,50,51,52,53,54,55,56,…”
Section: Introductionmentioning
confidence: 99%
“…Fig. 10 shows predicted neutron and proton elliptic flows in Au + Au reaction under the FOPI-LAND experimental conditions (here we use the data with b = 7.2 fm case) and geometry [20]. The experimental data was multiplied by a factor 1.15 owing to dispersion of the reaction plane [55].…”
Section: Resultsmentioning
confidence: 99%
“…To unscramble symmetry energy related experimental data, various isospin-dependent transport models are frequently used to probe the symmetry energy below and above saturation density [1,2]. With great efforts, the nuclear symmetry energy and its slope around saturation density of nuclear matter from 28 analysis of terrestrial nuclear laboratory experiments and astrophysical observations have been roughly pinned down [15], while recent interpretations of the FOPI and FOPI-LAND experimental measurements by different groups made the symmetry energy at supra-saturation densities fall into chaos [16][17][18][19][20][21][22]. It does not seem to be clarified why the nuclear symmetry energy at supra-saturation densities is so uncertain, maybe the effects of pion inmedium effects [23][24][25], the isospin dependence of inmedium nuclear strong interactions [26], the short-range tensor force [27,28] are some factors.…”
Section: Introductionmentioning
confidence: 99%
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“…Among the potential probes of the high-density symmetry energy, the π − /π + ratio in heavy-ion collisions has attracted much attention since it was first proposed [12]. Unfortunately, several model analyses [13][14][15][16][17][18] of some existing data have so far been inconclusive. Realizing the importance of thoroughly understanding all aspects of the π − N − ∆ dynamics in isospin-asymmetric matter especially since several experiments measuring the π − /π + ratio are cur- * Email: Bao-An.Li@Tamuc.edu rently underway at RIKEN [19] and NIRS [20] besides those planned at other facilities [21,22], significant efforts have been made recently in studying effects of the in-medium pion production threshold [23], pion meanfield [24][25][26][27], electromagnetic field [28], neutron-skin [29] and nucleon-nucleon short-range correlation [30,31] on pion production mostly at intermediate energies above the pion production threshold of about 300 MeV/A.…”
Section: Introductionmentioning
confidence: 99%