Photoproduction of gravitational radiation by pulsars

Details Photoproduction of gravitational radiation by pulsars Photoproduction of gravitational radiation by pulsars

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975cajph..53.2312p&link_type=abstract

Canadian Journal of Physics, vol. 53, Oct. 15, 1975, p. 2312-2314. Research supported by the National Research Council of Canad

Physics

4

Field Emission, Gravitational Waves, Gravitons, Neutron Stars, Photoproduction, Pulsars, Dipole Moments, Electromagnetic Fields, Particle Production, Quadrupoles

Scientific paper

Emission of gravitational radiation via photoproduction in static electromagnetic fields can equal or exceed the quadrupole contribution for pulsars whose ellipticity is less than 0.001 and may play a role in the cooling of the star. Contrary to the quadrupole emission case, radiation can take place also when the direction of the dipole moment and the rotation axis coincide. Radiation rates are also estimated for several frequency ranges of the photon spectrum.

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