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• W2078709724 abstract "Abstract 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." @default.
• W2078709724 created "2016-06-24" @default.
• W2078709724 creator A5049052946 @default.
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• W2078709724 date "1981-10-01" @default.
• W2078709724 modified "2023-09-24" @default.
• W2078709724 title "Is collapse of a deformed star always effectual for gravitational radiation?" @default.
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• W2078709724 doi "https://doi.org/10.1016/0370-2693(81)91082-0" @default.
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