Constraints on Non-Radial Oscillation Modes by Symmetry Energy Slope

The effect of the nuclear symmetry energy slope on the non-radial oscillation f-modes in neutron stars is calculated and discussed. Based on a conservative range of the symmetry energy slope constrained by the experiment and theoretical analysis, a constraint on the frequency and damping time of the...

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Bibliographic Details
Published inCommunications in theoretical physics Vol. 61; no. 4; pp. 469 - 474
Main Author 周颖 文德华
Format Journal Article
LanguageEnglish
Published 01.04.2014
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