Evolution of small-mass-ratio binaries with a spinning secondary - INSPIRE

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Evolution of small-mass-ratio binaries with a spinning secondary

Niels Warburton
(
- University Coll., Dublin
)
,
Thomas Osburn
(
- Oxford U.
)
,
Charles R. Evans
(
- North Carolina U.
)

Aug 11, 2017

17 pages

Published in:

Phys.Rev.D 96 (2017) 8, 084057

Published: Oct 26, 2017

e-Print:

1708.03720 [gr-qc]

DOI:

10.1103/PhysRevD.96.084057

View in:

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Abstract: (APS)

We calculate the evolution and gravitational-wave emission of a spinning compact object inspiraling into a substantially more massive (nonrotating) black hole. We extend our previous model for a nonspinning binary [Phys. Rev. D 93, 064024 (2016)PRVDAQ2470-001010.1103/PhysRevD.93.064024] to include the Mathisson-Papapetrou-Dixon spin-curvature force. For spin-aligned binaries we calculate the dephasing of the inspiral and associated waveforms relative to models that do not include spin-curvature effects. We find this dephasing can be either positive or negative depending on the initial separation of the binary. For binaries in which the spin and orbital angular momentum are not parallel, the orbital plane precesses and we use a more general osculating element prescription to compute inspirals.

Note:

17 pages, 6 figures

04.30.-w
04.25.Nx
04.30.Db
gravitational radiation: emission
binary: coalescence
orbit
precession
angular momentum
black hole
spin

References(126)

Figures(6)

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(
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)
,
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(
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)
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)
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)
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Stanislav Babak
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)
,
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)
,
Jonathan R. Gair
(
- Cambridge U.
)
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)
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Scott A. Hughes
(
- MIT and
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)

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)

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[24]

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Leor Barack
(
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)
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Norichika Sago
(
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)

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