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Emission of Gravitational Waves from the Pulsar

Published online by Cambridge University Press:  07 February 2017

R. Ruffini
R. Ruffini*
Affiliation:
Institute for Advance Study, School of Natural Sciences, Princeton, N.J., U.S.A.

Extract

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Dr. Ruffini gave a brief survey of the present experimental evidence for the existence of gravitational waves, and discussed the possibility that the shapes of neutron stars might depart from rotational symmetry, leading to the emission of gravitational waves.

Type
Session 6
Information
Symposium - International Astronomical Union , Volume 46: The Crab Nebula , 1971 , pp. 382 - 383
Copyright
Copyright © Reidel 1971