Gravitational-Wave Astronomy with Inspiral Signals of Spinning Compact-Object Binaries

Document #:

LIGO-P070107-x0

Document type:

P - Publications

Abstract:

Inspiral signals from binary compact objects (black holes and neutron stars) are primary targets of the ongoing searches by ground-based gravitational-wave interferometers (LIGO, Virgo, and GEO-600). We present parameter-estimation simulations for inspirals of black hole-neutron star binaries using Markov Chain Monte Carlo methods. For the first time, we both estimated the parameters of a binary inspiral source with a spinning, precessing component and determined the accuracy of the parameter estimation, for simulated observations with ground-based gravitational-wave detectors. We demonstrate that we can obtain the distance, sky position, and binary orientation at a higher accuracy than previously suggested in the literature. For an observation of an inspiral with sufficient spin and two or three detectors we find an accuracy in the determination of the sky position of the order of tens of square degrees.

Files in Document:

• P070107-00.pdf (file is not accessible)

Other Files:

• P070107-P.pdf (file is not accessible)

Topics:

• Document Migration from the old DCC
• Public relations

Authors:

• Vivien Raymond
• Marc van der Sluys
• Vassiliki Kalogera
• Nelson Christensen
• Alberto Vecchio
• Ilya Mandel
• Christian Roever
• Alexander Stroeer
• Renate Meyer

Notes and Changes:

Rev P070107-00-Z:
- Full document number: LIGO-P070107-00-Z
- Author(s): Marc Van Der Sluys; Christian Rover; A. Stroeer; Nelson Christensen; Vassiliki Kalogera; Renate Meyer; Alberto Vecchio
- Document date: 2007-09-24
- Document received date: 2007-09-26
- Document entry date: 2007-09-26

Journal References:

Published in ApJ Letters vol. 688 pg. L61-L64.

Publication Information:

http://www.iop.org/EJ/abstract/1538-4357/688/2/L61