Analytic properties of the electromagnetic field of binary compact stars and electromagnetic precursors to gravitational waves
Abstract We analytically study the properties of the electromagnetic field in the vacuum around close binary compact stars containing at least one neutron star. We show that the orbital motion of the neutron star induces high multipole modes of the electromagnetic field just before the merger. These...
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Published in | Progress of theoretical and experimental physics Vol. 2020; no. 10 |
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Format | Journal Article |
Language | English |
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01.10.2020
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Abstract | Abstract
We analytically study the properties of the electromagnetic field in the vacuum around close binary compact stars containing at least one neutron star. We show that the orbital motion of the neutron star induces high multipole modes of the electromagnetic field just before the merger. These modes are superimposed to form a spiral arm configuration, and its edge is found to be a likely site for magnetic reconnection. These modes also enhance the total Poynting flux from neutron star binaries by a factor of 2–4. We also indicate that the electric field induced by the orbital motion leads to a magnetosphere around binaries and estimate its plasma density, which has a different parameter dependence than the Goldreich–Julian density. With these properties, we discuss possible electromagnetic counterparts to gravitational wave events, and identify radio precursors, such as fast radio bursts, as the most promising observational targets. |
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AbstractList | We analytically study the properties of the electromagnetic field in the vacuum around close binary compact stars containing at least one neutron star. We show that the orbital motion of the neutron star induces high multipole modes of the electromagnetic field just before the merger. These modes are superimposed to form a spiral arm configuration, and its edge is found to be a likely site for magnetic reconnection. These modes also enhance the total Poynting flux from neutron star binaries by a factor of 2–4. We also indicate that the electric field induced by the orbital motion leads to a magnetosphere around binaries and estimate its plasma density, which has a different parameter dependence than the Goldreich–Julian density. With these properties, we discuss possible electromagnetic counterparts to gravitational wave events, and identify radio precursors, such as fast radio bursts, as the most promising observational targets. Abstract We analytically study the properties of the electromagnetic field in the vacuum around close binary compact stars containing at least one neutron star. We show that the orbital motion of the neutron star induces high multipole modes of the electromagnetic field just before the merger. These modes are superimposed to form a spiral arm configuration, and its edge is found to be a likely site for magnetic reconnection. These modes also enhance the total Poynting flux from neutron star binaries by a factor of 2–4. We also indicate that the electric field induced by the orbital motion leads to a magnetosphere around binaries and estimate its plasma density, which has a different parameter dependence than the Goldreich–Julian density. With these properties, we discuss possible electromagnetic counterparts to gravitational wave events, and identify radio precursors, such as fast radio bursts, as the most promising observational targets. |
Author | Wada, Tomoki Ioka, Kunihito Shibata, Masaru |
Author_xml | – sequence: 1 givenname: Tomoki surname: Wada fullname: Wada, Tomoki email: tomoki.wada@yukawa.kyoto-u.ac.jp organization: Center for Gravitational Physics, Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto, 606-8502, Japan – sequence: 2 givenname: Masaru surname: Shibata fullname: Shibata, Masaru organization: Center for Gravitational Physics, Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto, 606-8502, Japan – sequence: 3 givenname: Kunihito surname: Ioka fullname: Ioka, Kunihito organization: Center for Gravitational Physics, Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto, 606-8502, Japan |
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We analytically study the properties of the electromagnetic field in the vacuum around close binary compact stars containing at least one neutron... We analytically study the properties of the electromagnetic field in the vacuum around close binary compact stars containing at least one neutron star. We show... |
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SubjectTerms | Black holes Electromagnetism Gamma rays Gravitational waves Magnetic fields Neutron stars Neutrons Physics Plasma Radiation Simulation Velocity |
Title | Analytic properties of the electromagnetic field of binary compact stars and electromagnetic precursors to gravitational waves |
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