Gravitational Radiation and Steady-State Distribution of Binary Orbits - Application to High-Mass Binary Pulsars

Details Gravitational Radiation and Steady-State Distribution of Binary Orbits - Application to High-Mass Binary Pulsars Gravitational Radiation and Steady-State Distribution of Binary Orbits - Application to High-Mass Binary Pulsars

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994mnras.268..841b&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 268, NO. 4/JUN15, P. 841, 1994

Astronomy and Astrophysics

Astronomy

6

Gravitation - Radiation Mechanisms: Non-Thermal - Binaries: Close - Pulsars: General

Scientific paper

By assuming the existence of a quasi-steady state of binary orbits of collapsed objects, a simple theory, relating the initial input distribution of semimajor axis and eccentricity to the steady-state distribution of these parameters, is formulated under the working hypothesis that the mechanism of variation of the above parameters is the emission of gravitational waves. In order to illustrate this, a plausible steady-state distribution for the case of high-mass binary pulsars is obtained.

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