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Inspiral waveforms for spinning compact binaries in a new precessing convention
It is customary to use a precessing convention, based on Newtonian orbital
angular momentum , to model inspiral gravitational waves from
generic spinning compact binaries. A key feature of such a precessing
convention is its ability to remove all spin precession induced modulations
from the orbital phase evolution. However, this convention usually employs a
post-Newtonian (PN) accurate precessional equation, appropriate for the PN
accurate orbital angular momentum , to evolve the -based precessing source frame. This motivated us to develop inspiral
waveforms for spinning compact binaries in a precessing convention that
explicitly use to describe the binary orbits. Our approach introduces
certain additional 3PN order terms in the orbital phase and frequency evolution
equations with respect to the usual -based implementation of
the precessing convention. The implications of these additional terms are
explored by computing the match between inspiral waveforms that employ and -based precessing conventions. We found that the match
estimates are smaller than the optimal value, namely 0.97, for a non-negligible
fraction of unequal mass spinning compact binaries.Comment: 4 pages, 1 figures, published in the proceedings of Amaldi 1
File Naming Convention Worksheet
This worksheet walks researchers through the process of creating a file naming convention for a group of files. This process includes: choosing metadata, encoding and ordering the metadata, adding version information, and properly formatting the file names. Two versions of the worksheet are available: a Caltech Library branded version and a generic editable version
Symmetric Space Sigma-model Dynamics: Internal Metric Formalism
For the symmetric space sigma model in the internal metric formalism we
explicitly construct the lagrangian in terms of the axions and the dilatons of
the solvable Lie algebra gauge and then we exactly derive the axion-dilaton
field equations.Comment: 10 page
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