An Observable Peculiarity of the Brans-Dicke Radiation Zone

Details An Observable Peculiarity of the Brans-Dicke Radiation Zone An Observable Peculiarity of the Brans-Dicke Radiation Zone

Feb 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969phrvl..22..198r&link_type=abstract

Physical Review Letters, vol. 22, Issue 5, pp. 198-200

Physics

5

Scientific paper

It is pointed out that the Brans-Dicke theory predicts a transverse spin-0 component of the O(r-1) radiative Riemann tensor. Unlike the conventional spin-2 radiative Riemann tensor, monopole oscillations may serve as a source. Under favorable conditions, neutron star formation within our galaxy will be detectable by Weber's gravitational-wave receiver.

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