GRAVITATIONAL RADIATION FROM HYDRODYNAMIC TURBULENCE IN A DIFFERENTIALLY ROTATING NEUTRON STAR
A Melatos, C Peralta
Astrophysical Journal | IOP PUBLISHING LTD | Published : 2010
The authors thank Ira Wasserman for privileged early access to an illuminating preprint (I.M. Wasserman 2009, private communication), Sterl Phinney for directing us to the work of Kosowsky and collaborators, Scott Hughes for a valuable discussion on multipole expansions, and the anonymous referee for spotting an error in our original calculation of the decoherence time and for generally improving the manuscript. We also acknowledge the substantial computing resources and support provided by the Victorian Partnership for Advanced Computing and the Damiana Cluster at the Albert-Einstein-Institut, which made the simulations in this paper possible. A. M. thanks the Astronomy Department at Cornell University and the LIGO Data Analysis Group at the California Institute of Technology for their hospitality during the period when this work began, and the LIGO Visitor Program for financial support. C. P. acknowledges the support of the Max-Planck Society (Albert-Einstein Institut).