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Response of a mechanical oscillator to a gravitational wave.

Authors :
Westervelt, Peter J.
Source :
Journal of the Acoustical Society of America; 1975, Vol. 57 Issue S1, pS30-S30, 1p
Publication Year :
1975

Abstract

The conventional treatment [J. Weber, General Relativity and Gravitational Waves (Interscience, New York, 1961)] of an undamped mass quadrupole oscillator driven by a gravitational wave assumes the excitation force to be that exerted by the wave on the mass. The force exerted by the wave on the spring has heretofore been ignored. I have calculated this latter force Fs driving the spring and discovered that it is related to the force Fm driving the mass; thus, <DFORMULA>F<subscript>m</subscript> = ω<subscript>0</subscript><superscript>-2</superscript> <FRACTION><NUM>d<superscript>2</superscript></NUM><DEN>dt<superscript>2</superscript></DEN></FRACTION> F<subscript>s</subscript></DFORMULA>, in which ω0 is the resonant circular frequency of the oscillator. The total driving force is the sum Fm + Fs. This total force is incapable of exciting the normal mode of the oscillator, thus supporting my earlier conjecture [P. J. Westervelt, Soviet Phys. JETP Letters 4, 225 (1966), Footnote 4] that passive detectors of gravitational waves cannot be realized in principle. Active detectors, i.e., generators of gravitational waves, can measure radiation from another source. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
00014966
Volume :
57
Issue :
S1
Database :
Complementary Index
Journal :
Journal of the Acoustical Society of America
Publication Type :
Academic Journal
Accession number :
75076923
Full Text :
https://doi.org/10.1121/1.1995166