Merging neutron stars generate Alfvén-wing current channels in the relativistic sub-Alfvénic regime, potentially producing beamed electromagnetic precursor emission before the gravitational-wave signal.
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Production of Jets before Neutron Star Mergers
Merging neutron stars generate Alfvén-wing current channels in the relativistic sub-Alfvénic regime, potentially producing beamed electromagnetic precursor emission before the gravitational-wave signal.