| 11. | Until then, their gravitational radiation would be comparable to that of a neutron star binary.
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| 12. | Physically, these represent purely gravitational radiation propagating along the null rays \ partial _ v.
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| 13. | Changing mass-current multipoles can also give off gravitational radiation.
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| 14. | :Strictly speaking the only non-electromagnetic radiation is gravitational radiation.
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| 15. | Angular momentum is also lost in the gravitational radiation.
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| 16. | Two neutron stars rotating rapidly around one another gradually lose energy by emitting gravitational radiation.
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| 17. | Relativity predicts that over time a binary system's orbital energy will be converted to gravitational radiation.
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| 18. | :: I think both of you are confusing gravitational fields with gravitational radiation ( waves ).
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| 19. | The mass quadrupole, however, can change in time, and is the lowest-order contribution to gravitational radiation.
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| 20. | Hessels goes on to speculate that gravitational radiation from the pulsar might be detectable by LIGO.
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