Is collapse of a deformed star always effectual for gravitational radiation?

Details Is collapse of a deformed star always effectual for gravitational radiation? Is collapse of a deformed star always effectual for gravitational radiation?

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981phlb..106...69n&link_type=abstract

Physics Letters B, Volume 106, Issue 1-2, p. 69-72.

Physics

34

Scientific paper

We have computed the energy of gravitational radiation from an axially symmetric, non-rotating dust shell of mass m falling into a Schwarzschild black hole of mass M >> m. Both prolate and oblate dust shells are examined. A strongly deformed dust shell radiates less gravitational waves than a moderately deformed one. The radiation energy from a dust shell is less than that from a test particle, which is contrary to the newtonian result of Thuan and Ostriker which did not take phase cancellation effects into account.

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