Dynamics of electromagnetic waves in Kerr geometry

@article{Mukhopadhyay2002DynamicsOE,
title={Dynamics of electromagnetic waves in Kerr geometry},
author={Banibrata Mukhopadhyay},
journal={arXiv: General Relativity and Quantum Cosmology},
year={2002}
}

Here we are interested to study the spin-1 particle i.e., electro-magnetic wave in curved space-time, say around black hole. After separating the equations into radial and angular parts, writing them according to the black hole geometry, say, Kerr black hole we solve them analytically. Finally we produce complete solution of the spin-1 particles around a rotating black hole namely in Kerr geometry. Obviously there is coupling between spin of the electro-magnetic wave and that of black hole when… Expand

Separation of the Dirac equation in the spacetime around a Kerr black hole into radial and angular coordinates was done by Chandrasekhar in 1976. In the present paper, we solve the radial equations… Expand

Separable wave equations with source terms are presented for electromagnetic and gravitational perturbations of an uncharged, rotating black hole. These equations describe the radiative field… Expand

Proceedings of the Royal Society of London. A. Mathematical and Physical Sciences

1984

The angular functions in Chandrasekhar’s separation of the variables of Dirac’s equation in Kerr geometry are solved by an expansion procedure based on spin-weighted spherical harmonics. The… Expand

Proceedings of the Royal Society of London. A. Mathematical and Physical Sciences

1976

Explicit solutions for the vector-potential of a vacuum Maxwell-field in Kerr geometry are obtained in terms of Teukolsky’s radial and angular functions.

OF THE DISCLOSURE A gas Spring for a drawing table which has a cylinder, a piston in the cylinder, and a piston rod projecting from the piston through one end wall of the cylinder, the other end wall… Expand