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Gravitational and electromagnetic outputs from binary neutron star mergers

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arxiv 1301.7074 v2 pith:C5VRDHHP submitted 2013-01-29 gr-qc astro-ph.HE

Carlos Palenzuela , Luis Lehner , Marcelo Ponce , Steven L. Liebling , Matthew Anderson , David Neilsen , Patrick Motl This is my paper · ORCID
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keywords binaryneutronstarelectromagneticgravitationalinteractionsmergerspower
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The late stage of an inspiraling neutron star binary gives rise to strong gravitational wave emission due to its highly dynamic, strong gravity. Moreover, interactions between the stellar magnetospheres can produce considerable electromagnetic radiation. We study this scenario using fully general relativistic, resistive magneto-hydrodynamics simulations. We show that these interactions extract kinetic energy from the system, dissipate heat, and power radiative Poynting flux, as well as develop current sheets. Our results indicate that this power can: (i) outshine pulsars in binaries, (ii) display a distinctive angular- and time-dependent pattern, and (iii) radiate within large opening angles. These properties suggest that some binary neutron star mergers are ideal candidates for multimessenger astronomy.

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    A binary black hole merger is visualized through gravitational electric and magnetic fields obtained from an exact Maxwell-like reformulation of general relativity.

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