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arXiv · 1212.5996

Merging neutron star binaries: equation of state and electrodynamics

Dong Lai
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Abstract

Merging neutron star (NS) binaries may be detected by ground-based gravitational wave (GW) interferometers (e.g. LIGO/VIRGO) within this decade and may also generate electromagnetic radiation detectable by wide-field, fast imaging telescopes that are coming online. The GWs can provide new constraint on the NS equation of state (including mass-radius relation and the related nuclear symmetry energy through resonant g-modes). This paper reviews various hydrodynamical (including equilibrium and dynamical/resonant tides) and electrodynamical processes in coalescing NS binaries, with focus on the pre-merger phase.

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Dong Lai. 2012-12-25. Merging neutron star binaries: equation of state and electrodynamics. https://doi.org/10.1017/s1743921312023459

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