2006
DOI: 10.1103/physrevc.73.037311
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Approximate analytical solution for nuclear matter in a mean-field Walecka model and Coester line behavior

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Cited by 4 publications
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“…Alternatively, DBHF calculations have been shown to be effective without the need for NNN forces [17,20]. Another possibility is to treat the scalar and vector densities in the Walecka relativistic mean-field model [21] as equal [22]. However, the systematic deviation of all theoretical predictions from the expected empirical values of E o and ρ o remains a problem.…”
Section: Introductionmentioning
confidence: 99%
“…Alternatively, DBHF calculations have been shown to be effective without the need for NNN forces [17,20]. Another possibility is to treat the scalar and vector densities in the Walecka relativistic mean-field model [21] as equal [22]. However, the systematic deviation of all theoretical predictions from the expected empirical values of E o and ρ o remains a problem.…”
Section: Introductionmentioning
confidence: 99%