Gravitationally driven electromagnetic perturbations of neutron stars and black holes

Hajime Sotani, Kostas D. Kokkotas, Pablo Laguna, and Carlos F. Sopuerta
Phys. Rev. D 87, 084018 – Published 5 April 2013

Abstract

Gravitational perturbations of neutron stars and black holes are well-known sources of gravitational radiation. If the compact object is immersed in or endowed with a magnetic field, the gravitational perturbations would couple to electromagnetic perturbations and potentially trigger synergistic electromagnetic signatures. We present a detailed analytic calculation of the dynamics of coupled gravitational and electromagnetic perturbations for both neutron stars and black holes. We discuss the prospects for detecting the electromagnetic waves in these scenarios and the potential that these waves have for providing information about their source.

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  • Received 15 February 2013

DOI:https://doi.org/10.1103/PhysRevD.87.084018

© 2013 American Physical Society

Authors & Affiliations

Hajime Sotani1, Kostas D. Kokkotas2,3, Pablo Laguna4, and Carlos F. Sopuerta5

  • 1Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-8502, Japan
  • 2Theoretical Astrophysics, University of Tübingen, IAAT, Auf der Morgenstelle 10, 72076 Tübingen, Germany
  • 3Department of Physics, Aristotle University of Thessaloniki, 54124 Thessaloniki, Greece
  • 4Center for Relativistic Astrophysics and School of Physics, Georgia Institute of Technology, Atlanta, Georgia 30332, USA
  • 5Facultat de Ciències, Institut de Ciències de l’Espai (CSIC-IEEC), Campus UAB, Torre C5 parells, Bellaterra, 08193 Barcelona, Spain

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Issue

Vol. 87, Iss. 8 — 15 April 2013

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