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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Published in | Communications in theoretical physics Vol. 61; no. 4; pp. 469 - 474 |
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Main Author | |
Format | Journal Article |
Language | English |
Published |
01.04.2014
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Subjects | |
Online Access | Get full text |
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