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A Double-Pulsar System - A Rare Laboratory for Relativistic Gravity and Plasma Physics

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arxiv astro-ph/0401086 v1 pith:CXP4PMSA submitted 2004-01-07 astro-ph

A Double-Pulsar System - A Rare Laboratory for Relativistic Gravity and Plasma Physics

A.G. Lyne , M. Burgay , M. Kramer , A. Possenti , R.N. Manchester , F. Camilo , M.A. McLaughlin , D.R. Lorimer
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N. D'Amico B.C. Joshi J. Reynolds P.C.C. Freire
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keywords gravitationalj0737-3039aj0737-3039bpulsarfluxmagnetospherephysicsproperties
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The clock-like properties of pulsars moving in the gravitational fields of their unseen neutron-star companions have allowed unique tests of general relativity and provided evidence for gravitational radiation. We report here the detection of the 2.8-sec pulsar J0737-3039B as the companion to the 23-ms pulsar J0737-3039A in a highly-relativistic double-neutron-star system, allowing unprecedented tests of fundamental gravitational physics. We observe a short eclipse of J0737-3039A by J0737-3039B and orbital modulation of the flux density and pulse shape of J0737-3039B, probably due to the influence of J0737-3039A's energy flux upon its magnetosphere. These effects will allow us to probe magneto-ionic properties of a pulsar magnetosphere.

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Cited by 2 Pith papers

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  1. The Southern-sky MWA Rapid Two-metre (SMART) pulsar survey--IV. Survey update and an atlas of 205 non-recycled southern pulsars

    astro-ph.HE 2026-07 accept novelty 6.0

    Atlas of 205 non-recycled southern pulsars at 140–170 MHz from MWA SMART data, with profiles, DMs, RMs, fluxes and public data products for SKA-Low.

  2. The Confrontation between General Relativity and Experiment

    gr-qc 2014-03 accept novelty 2.0

    Experiments confirm general relativity to high precision in weak-field and strong-field regimes, with gravitational wave damping matching predictions to better than 0.5 percent.