Gravitational Radiation from Pulsating White Dwarfs

Details Gravitational Radiation from Pulsating White Dwarfs Gravitational Radiation from Pulsating White Dwarfs

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aps..nws.b1008b&link_type=abstract

American Physical Soceity, Fifth Annual Meeting of the Northwest Section Meeting, May 30-31, 2003, Reed college, Portland, Orego

Physics

Scientific paper

Rotating white dwarfs undergoing quasi-radial oscillations can emit gravitational radiation in a frequency range from 0.1 - 1 Hz. Assuming that the energy source for the gravitational radiation comes from the oblateness of the white dwarf induced by the rotation, the strain amplitude is found to be ˜ 10^27 for a white dwarf at 10 pc. The galactic population of these sources may be observable by future interferometric detectors operating in the decihertz band.

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