Tilted torus magnetic fields in neutron stars and their gravitational wave signatures
Paul D Lasky, Andrew Melatos
Physical Review D | AMER PHYSICAL SOC | Published : 2013
Awarded by Australian Research Council
We are grateful to Alpha Mastrano and Sam Lander for valuable discussions, and to Anton Tarasenko for an early implementation of the moment of inertia calculations within the HORIZON code. P. D. L. is especially grateful to Burkhard Zink and Kostas Kokkotas for work and discussions related to the HORIZON code. We thank the anonymous referee for insightful feedback that has improved the manuscript. This work is supported by an Australian Research Council Discovery Project Grant No. (DP110103347). P. D. L. is supported by an internal University of Melbourne Early Career Researcher Grant. The numerical simulation was performed on the Multimodal Australian ScienceS Imaging and Visualisation Environment (MASSIVE; www.massive.org.au) through an award under the Merit Allocation Scheme on the NCI National Facility at the ANU.