On the linearization of Maxwell equations in the field of a weak gravitational wave

1985 ◽  
Vol 162 (1) ◽  
pp. 49-52 ◽  
Author(s):  
L. Baroni ◽  
P. Fortini ◽  
C. Gualdi
2016 ◽  
Vol 55 (9) ◽  
pp. 4100-4108
Author(s):  
F. Tavakoli ◽  
R. Pirmoradian ◽  
I. Parsabod

1995 ◽  
Vol 04 (02) ◽  
pp. 207-213
Author(s):  
N.I. KOLOSNITSYN

Conversion of a gravitational wave into an electromagnetic one in a laser coherent emission field is studied. As a result two electromagnetic waves are created. For calculation the Maxwell equations in three-dimensional vector form are used. Optimal detection of the gravitational wave is discussed. In a particular case it is the laser interferometric antenna. This approach is identical to those based on integration of the isotropic geodesic equation, the eikonal equation, giving the three-pulsing response of the electromagnetic signal obtained by Estabrook and Wahlquist. It also results in the matrix method developed by Vinet for calculation of laser interferometric antennae.


2017 ◽  
Vol 95 (10) ◽  
Author(s):  
Donato Bini ◽  
Andrea Geralico ◽  
Antonello Ortolan

1974 ◽  
Vol 64 ◽  
pp. 59-59
Author(s):  
V. DE SABBATA ◽  
P. Fortini ◽  
C. Gualdi ◽  
L. Fortini Baroni

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.


1997 ◽  
Vol 40 (8) ◽  
pp. 717-720
Author(s):  
V. I. Babetskii ◽  
G. N. Izmailov

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