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Radio and X-ray Signatures of Merging Neutron Stars

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arxiv astro-ph/0003218 v1 pith:AQPZ2XKM submitted 2000-03-15 astro-ph

classification astro-ph
keywords possibleradiosignalsx-raydescribeneutronbinarybursts
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We describe the possible electromagnetic signals expected from the magnetospheric interactions of a neutron star binary prior to merger. We find that both radio and X-ray signals of detectable strength are possible. We discuss possible links with the phenomenon of gamma-ray bursts and describe the prospects for direct detection of these signals in searches for radio and X-ray transients.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Cherenkov emission by a fast-moving uncharged Schwarzschild black hole

    hep-th 2025-02 conditional novelty 8.0 of 10

    An uncharged Schwarzschild black hole moving superluminally through a dielectric in a magnetic field is predicted to emit classical Cherenkov radiation via gravity-distorted field lines.

  2. Empirical Modeling of Magnetic Braking in Millisecond Pulsars to Measure the Local Dark Matter Density and Effects of Orbiting Satellite Galaxies

    astro-ph.HE 2025-01 conditional novelty 6.0 of 10

    A spin-down based empirical model for magnetic braking doubles the sample of pulsar acceleration measurements and yields a direct local dark matter density of 0.0098 +/- 0.0025 solar masses per cubic parsec.

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