Monday, October 15, 2012

1210.3402 (F. J. Fattoyev et al.)

Constraining the High-Density Behavior of Nuclear Symmetry Energy with
the Tidal Polarizability of Neutron Stars
   [PDF]

F. J. Fattoyev, J. Carvajal, W. G. Newton, Bao-An Li
Using a set of model equations of state satisfying the latest constraints from both terrestrial nuclear experiments and astrophysical observations as well as state-of-the-art nuclear many-body calculations of the pure neutron matter equation of state, the tidal polarizability of canonical neutron stars in coalescing binaries is found to be a very sensitive probe of the high-density behavior of nuclear symmetry energy which is among the most uncertain properties of dense neutron-rich nucleonic matter. Moreover, it changes less than $\pm 10%$ by varying various properties of symmetric nuclear matter and symmetry energy around the saturation density within their respective ranges of remaining uncertainty.
View original: http://arxiv.org/abs/1210.3402

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