On secular effects in the binary pulsar

Details On secular effects in the binary pulsar On secular effects in the binary pulsar

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.207p..37s&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 207, March 15, 1984, p. 37P-39P.

Astronomy and Astrophysics

Astronomy

1

Binary Stars, Equations Of Motion, Long Term Effects, Pulsars, Einstein Equations, Momentum

Scientific paper

The author shows that a recent suggestion by Lapiedra, Portilla & Sanz, that casts doubt on present interpretation of the binary pulsar observations, is incorrect. In particular, their suggestion that, if the binary system is moving relative to us then there will be a long-period modulation of its observed period, violates special relativity near the observer. In order to explain how the error in their conclusion arises, the author gives a detailed discussion of the correspondence between observable quantities and various Newtonian and post-Newtonian constructs.

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