Gravitational-wave chirps: accumulating phase errors due to residual orbital eccentricity View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

1996-11

AUTHORS

V. Pierro, I. M. Pinto

ABSTRACT

We compute to lowest order the phase error due to the circular-orbit assumption in modelling gravitational-wave chirps from coalescing binaries. The error increases steeply as one proceeds toward coalescence, and can be comparable to π even for very small (residual) initial orbital eccentricities, thus deteriorating severely the detector’s performance.

PAGES

1517-1525

References to SciGraph publications

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/bf02741491

DOI

http://dx.doi.org/10.1007/bf02741491

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1024857975


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