Loss of angular momentum in a binary system due to collisionless particles as monopoles or gravitinos - Does it exceed the gravitational radiation emission in the binary system PSR 1913+16?

Details Loss of angular momentum in a binary system due to collisionless particles as monopoles or gravitinos - Does it exceed the gravitational radiation emission in the binary system PSR 1913+16? Loss of angular momentum in a binary system due to collisionless particles as monopoles or gravitinos - Does it exceed the gravitational radiation emission in the binary system PSR 1913+16?

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nciml..36..449f&link_type=abstract

Nuovo Cimento, Lettere, Serie 2, vol. 36, April 2, 1983, p. 449-452.

Computer Science

4

Angular Momentum, Binary Stars, Celestial Mechanics, Gravitational Waves, Gravitinos, Magnetic Monopoles, Pulsars, Collisionless Plasmas, Energy Dissipation, Particle Density (Concentration), Solar Corpuscular Radiation, Stellar Gravitation, Wave Drag

Scientific paper

The gravitational drag for a massive object moving in the nearly collisiondess fluid made by magnetic monopoles is examined. It is shown that for a known binary system in our Galaxy associated with pulsar PSR 1913+16, a monopole number density larger than the expected solar value of 10 to the -7th/cu cm may induce an energy loss comparable or even larger than the one due to the gravitational radiation of the system. It is concluded that this drag mechanism may be a relevant test for detecting indirectly the presence of a collisionless cloud in a binary system and it may be used to infer some limits on the magnetic monopole density near the sun.

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