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 inProgress of theoretical and experimental physics Vol. 2020; no. 10
Main Authors Wada, Tomoki, Shibata, Masaru, Ioka, Kunihito
Format Journal Article
LanguageEnglish
Published Oxford Oxford University Press 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.
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
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  givenname: Masaru
  surname: Shibata
  fullname: Shibata, Masaru
  organization: Center for Gravitational Physics, Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto, 606-8502, Japan
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  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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Snippet Abstract 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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