2016
DOI: 10.1103/physrevc.94.054602
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Astrophysical S factor for the Li6(d,α)4He and

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Cited by 7 publications
(9 citation statements)
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“…We may, therefore, expect that the effect of a strong magnetic field on the transition will also depend on the symmetry energy, since the magnetic field is sensitive to the amount of protons: the smaller the proton density, the stronger are the effects. In previous studies [12,13], this aspect has already been identified.…”
Section: Symmetry Energy Effectmentioning
confidence: 56%
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“…We may, therefore, expect that the effect of a strong magnetic field on the transition will also depend on the symmetry energy, since the magnetic field is sensitive to the amount of protons: the smaller the proton density, the stronger are the effects. In previous studies [12,13], this aspect has already been identified.…”
Section: Symmetry Energy Effectmentioning
confidence: 56%
“…Above B * ∼ 10 3 (B ∼ 5 × 10 16 G), the AMM has a non-negligible effect and, therefore, we will essentially restrict ourselves to values below that number. As discussed in [12,13], the spinodal section shows a complex structure and bands of instability with large isospin asymmetry appear associated with the filling of the different Landau levels. As a result for low temperatures, the β-equilibrium EoS crosses the spinodal section several times, defining the region of instability referred before, see Fig.…”
Section: Symmetry Energy Effectmentioning
confidence: 93%
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