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Gravitational radiation from strongly magnetized white dwarfs
Authors:Jeremy S Heyl
Institution:Theoretical Astrophysics 130–33, California Institute of Technology, Pasadena, CA 91125, USA
Abstract:The magnetic fields of white dwarfs distort their shape generating an anisotropic moment of inertia. A magnetized white dwarf that rotates obliquely relative to the symmetry axis has a mass quadrupole moment that varies in time, so it will emit gravitational radiation. The Laser Interferometer Space Antenna ( LISA ) mission may be able to detect the gravitational waves from two nearby, rapidly rotating white dwarfs.
Keywords:gravitation  binaries: close  stars: magnetic fields  novae  cataclysmic variables  white dwarfs
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