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Interaction of Gravitational Radiation with a Uniformly Magnetized Sphere

Published online by Cambridge University Press:  07 February 2017

V. DE SABBATA ,
P. Fortini ,
C. Gualdi  and
L. Fortini Baroni
V. DE SABBATA
Affiliation:
Istituto di Fisica dell'Università Bologna, Bologna, Italy
P. Fortini
Affiliation:
Istituto di Fisica dell'Università Bologna, Bologna, Italy
C. Gualdi
Affiliation:
Istituto di Fisica dell'Università Bologna, Bologna, Italy
L. Fortini Baroni
Affiliation:
Holder of a C.N.R. ‘Italian National Research Council’ Scholarship, Bologna, Italy

Abstract

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Maxwell equations in the field of a gravitational wave are linearized by means of the weak field approximation. Then the equations are solved in the case of a uniformly magnetized sphere and the dipole electromagnetic radiation power is calculated. These results are applied to compute the electromagnetic radiation emitted by magnetic neutron stars and by the Earth when hit by gravitational radiation.

Type
Part I: Gravitational Radiation
Information
Symposium - International Astronomical Union , Volume 64: Gravitational Radiation and Gravitational Collapse , 1974 , pp. 59
Copyright
Copyright © Reidel 1974