Share Email Print

Proceedings Paper

A new method for estimating binary pulsar coalescence rates
Author(s): Vicky Kalogera; Chunglee Kim; Duncan R. Lorimer
Format Member Price Non-Member Price
PDF $14.40 $18.00
cover GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. Check Access

Paper Abstract

Estimates of the Galactic coalescence rate (R) of close binaries with two neutron stars (NS-NS) are known to be uncertain by large factors (about two orders of magnitude) mainly due to the small number of systems detected as binary radio pulsars. We present an analysis method that allows us to estimate the Galactic NS-NS coalescence using the current observed sample and, importantly, to assign a statistical significance to these estimates and to calculate the allowed ranges of values at various confidence levels. The method involves the simulation of selection effects inherent in all relevant radio pulsar surveys and a Bayesian statistical analysis for the probability distribution of R. The most likely values for the total Galactic coalescence rate (Rtot) lie in the range 2-60 Myr-1 depending on different pulsar population models. For our reference model 1, where the most likely estimates of pulsar population properties are adopted, we obtain Rtot = 8-5+9 Myr-1 at a 68% statistical confidence level. The corresponding range of expected detection rates of NS-NS inspiral are 3-2+4 × 10-3 yr-1 for the initial LIGO and 18-11+21 yr-1 for the advanced LIGO.

Paper Details

Date Published: 26 February 2003
PDF: 12 pages
Proc. SPIE 4856, Gravitational-Wave Detection, (26 February 2003); doi: 10.1117/12.458969
Show Author Affiliations
Vicky Kalogera, Northwestern Univ. (United States)
Chunglee Kim, Northwestern Univ. (United States)
Duncan R. Lorimer, Jodrell Bank Observatory/Univ. of Manchester (United Kingdom)

Published in SPIE Proceedings Vol. 4856:
Gravitational-Wave Detection
Peter Saulson; Adrian M. Cruise, Editor(s)

© SPIE. Terms of Use
Back to Top