The Electromagnetic Christodoulou Memory Effect in Neutron Star Binary Mergers
Lydia Bieri, PoNing Chen, Shing-Tung Yau

TL;DR
This paper investigates the electromagnetic contribution to the nonlinear gravitational wave memory effect in neutron star mergers, showing it enhances the signal detected by interferometers and aids in understanding the source energy.
Contribution
It extends previous work by computing the electromagnetic Christodoulou memory effect specifically for neutron star mergers, linking electromagnetic fields to gravitational wave observations.
Findings
Electromagnetic fields significantly contribute to the nonlinear memory effect.
The electromagnetic contribution can enlarge the gravitational wave signal in detectors.
Results help estimate energy radiated in neutron star mergers.
Abstract
Gravitational waves are predicted by the general theory of relativity. In [6] D. Christodoulou showed that gravitational waves have a nonlinear memory. We proved in [3] that the electromagnetic field contributes at highest order to the nonlinear memory effect of gravitational waves. In the present paper, we study this electromagnetic Christodoulou memory effect and compute it for binary neutron star mergers. These are typical sources of gravitational radiation. During these processes, not only mass and momenta are radiated away in form of gravitational waves, but also very strong magnetic fields are produced and radiated away. Thus the observed effect on test masses of a laser interferometer gravitational wave detector will be enlarged by the contribution of the electromagnetic field. Therefore, the present results are important for the planned experiments. Looking at the null…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Stellar, planetary, and galactic studies · Nuclear Physics and Applications
