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No GW is emitted by B PSR1913+16

2005/02/16 by A. Loinger, Loinger, A. · 1 citation
Earth and Planetary Sciences · Physics and Astronomy · #Astro and Planetary Science #Geophysics and Gravity Measurements #Pulsars and Gravitational Waves Research #physics.gen-ph

paper · pdf · doi:10.48550/arxiv.physics/0502089

5 pages, LaTeX, to be published on Spacetime & Substance

arxiv created 2005/02/16 · arxiv updated 2009/12/01

Abstract

In the exact (non-linear) formulation of general relativity (GR) no motion of bodies can give origin to gravitational waves (GW's) - as it has been proved. Accordingly, the measured rate of change of the orbital period of binary pulsar B PSR1913+16 must have other causes, different from the emission of GW's; maybe the viscous losses of the unseen pulsar companion, if it were e.g. a helium star.

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