Summary
It is shown that the secular change of the total gravitational mass of a system of two bodies, uniformly rotating around each other, is exactly equal to minus the radiated energy (independently computed in the previous part of this paper).
Riassunto
Si dimostra che la variazione secolare della massa gravitazionale totale di un sistema di due corpi rotanti uniformemente uno attorno all’altro è esattamente uguale all’energia irradiata cambiata di segno (calcolata indipendentemente nella prima parte del presente lavoro).
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References
A. Peres:Nuovo Cimento 11, 644 (1959), hereafter refered to as II. All notations thoughout the present paper are those of II.
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Partly supported by the U.S. Air Force, through the Air Research and Development Command.
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Peres, A. Gravitational motion and radiation - III. Nuovo Cim 13, 439–441 (1959). https://doi.org/10.1007/BF02732954
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DOI: https://doi.org/10.1007/BF02732954