Gravitational wave emission from the coalescence of white dwarfs

Details Gravitational wave emission from the coalescence of white dwarfs Gravitational wave emission from the coalescence of white dwarfs

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005cqgra..22s.453g&link_type=abstract

Classical and Quantum Gravity, Volume 22, Issue 10, pp. S453-S456 (2005).

Computer Science

Scientific paper

We have computed the gravitational wave emission arising from the coalescence of several close white dwarf binary systems. In order to do so, we have followed the evolution of such systems using a smoothed particle hydrodynamics code. Here we present some of the results obtained so far, paying special attention to the detectability of the emitted gravitational waves. Within this context, we show which could be the impact of individual merging episodes for LISA.

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