Gravitational radiation from a rotating magnetic dipole
Shahen Hacyan
TL;DR
This paper calculates the gravitational radiation emitted by a rotating magnetic dipole, providing formulas for polarization and power, and compares it with other astrophysical sources like neutron stars.
Contribution
It introduces closed-form formulas for gravitational radiation from rotating magnetic dipoles and compares these with emissions from neutron stars.
Findings
Derived formulas for polarization amplitudes and radiated power.
Compared gravitational radiation from magnetic dipoles with neutron star emissions.
Highlighted potential significance in astrophysical contexts.
Abstract
The gravitational radiation emitted by a rotating magnetic dipole is calculated. Formulas for the polarization amplitudes and the radiated power are obtained in closed forms. A comparison is made with other sources of gravitational and electromagnetic radiation, particularly neutron stars with extremely powerful magnetic fields.
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Geophysics and Sensor Technology · Geophysics and Gravity Measurements