Self-interaction spin effects in inspiralling compact binaries - INSPIRE

DataBETA

Self-interaction spin effects in inspiralling compact binaries

Apr, 2005

Published in:

Phys.Rev.D 71 (2005) 124043

e-Print:

astro-ph/0504538 [astro-ph]

DOI:

10.1103/PhysRevD.71.124043

View in:

ADS Abstract Service

reference search166 citations

Citations per year

Abstract: (arXiv)

Gravitational radiation drives compact binaries through an inspiral phase towards a final coalescence. For binaries with\textit{spin, mass quadrupole and magnetic dipole moments}, various contributions add to this process, which is characterized by the rate of increase

df/dt

of the gravitational wave frequency and the accumulated number

\mathcal{N}

of gravitational wave cycles. We present here all contributions to

df/dt

and

% \mathcal{N}

up to the second post-Newtonian order. Among them we give for the first time the contributions due to the \textit{self-interaction of individual spins}. These are shown to be commensurable with the proper spin-spin contributions for the recently discovered J0737-3039 double pulsar, and argued to represent the first corrections to the radiation reaction in the Lense-Thirring approach.

04.25.Nx
04.30.Db

References(46)

Figures(0)

LIGO: The Laser interferometer gravitational wave observatory

Alex Abramovici
(
- Caltech and
- Caltech, JPL and
- MIT, LNS
)
,
William E. Althouse
(
- Caltech and
- Caltech, JPL and
- MIT, LNS
)
,
Ronald W.P. Drever
(
- Caltech and
- Caltech, JPL and
- MIT, LNS
)
,
Yekta Gursel
(
- Caltech and
- Caltech, JPL and
- MIT, LNS
)
,
Seiji Kawamura
(
- Caltech and
- Caltech, JPL and
- MIT, LNS
)

et al.

- Science 256 (1992) 325-333
•
DOI:
- 10.1126/science.256.5055.325

The Virgo Project: A Wide Band Antenna for Gravitational Wave Detection

A. Giazotto
(
- INFN, Pisa
)

- Nucl.Instrum.Meth.A 289 (1990) 518-525,
- In *Cavalese 1988, Proceedings, General relativity and gravitational physics* 221-237.
•
DOI:
- 10.1016/0168-9002(90)91525-G

Limits on gravitational wave emission from selected pulsars using LIGO data

LIGO Scientific

Collaboration

•

B. Abbott
(
- LIGO Lab., Caltech
)

et al.

- Phys.Rev.Lett. 94 (2005) 181103
•
e-Print:
- gr-qc/0410007
•
DOI:
- 10.1103/PhysRevLett.94.181103

Report on the first binary black hole inspiral search in LIGO data

LIGO Scientific

Collaboration

•

Eirini Messaritaki
(
- Wisconsin U., Milwaukee
)

for the collaboration.

- Class.Quant.Grav. 22 (2005) 18, S1119-S1128
•
e-Print:
- gr-qc/0504065
•
DOI:
- 10.1088/0264-9381/22/18/S26

Low frequency sources of gravitational waves: A Tutorial

Bernard F. Schutz
(
- Potsdam, Max Planck Inst. and
- Cardiff U.
)

- ESA Spec.Publ. 420 (1997) 229
•
e-Print:
- gr-qc/9710079

Estimating spinning binary parameters and testing alternative theories of gravity with LISA

- Phys.Rev.D 71 (2005) 084025
•
e-Print:
- gr-qc/0411129
•
DOI:
- 10.1103/PhysRevD.71.084025

Last orbits of binary strange quark stars

Francois Limousin
(
- LUTH, Meudon
)
,
Dorota Gondek-Rosinska
(
- LUTH, Meudon
)
,
Eric Gourgoulhon
(
- LUTH, Meudon
)

- Phys.Rev.D 71 (2005) 064012
•
e-Print:
- gr-qc/0411127
•
DOI:
- 10.1103/PhysRevD.71.064012

Impact of the nuclear equation of state on the last orbits of binary neutron stars

M. Bejger
(
- Warsaw, Copernicus Astron. Ctr.
)
,
D. Gondek-Rosinska
(
- Warsaw, Copernicus Astron. Ctr. and
- LUTH, Meudon
)
,
Eric Gourgoulhon
(
- LUTH, Meudon
)
,
P. Haensel
(
- Warsaw, Copernicus Astron. Ctr. and
- LUTH, Meudon
)
,
K. Taniguchi
(
- Tokyo U., Earth Sci. Dept. and
- Tokyo U., Astron. Dept.
)

et al.

- Astron.Astrophys. 431 (2005) 297
•
e-Print:
- astro-ph/0406234
•
DOI:
- 10.1051/0004-6361:20041441

The Influence of quark matter at high densities on binary neutron star mergers

- Mon.Not.Roy.Astron.Soc. 349 (2004) 1469
•
e-Print:
- astro-ph/0401083
•
DOI:
- 10.1111/j.1365-2966.2004.07621.x

Approximate matching of analytic and numerical solutions for rapidly rotating neutron stars

Emanuele Berti
(
- Thessaloniki U. and
- McDonnell Ctr. Space Sci.
)
,
Nikolaos Stergioulas
(
- Thessaloniki U.
)

- Mon.Not.Roy.Astron.Soc. 350 (2004) 1416
•
e-Print:
- gr-qc/0310061
•
DOI:
- 10.1111/j.1365-2966.2004.07740.x

Computing the merger of black hole binaries: The IBBH problem

- Phys.Rev.D 58 (1998) 061501
•
e-Print:
- gr-qc/9804057
•
DOI:
- 10.1103/PhysRevD.58.061501

Detection template families for gravitational waves from the final stages of binary--black-hole inspirals: Nonspinning case

Alessandra Buonanno
(
- Paris, Inst. Astrophys. and
- Caltech
)
,
Yan-bei Chen
(
- Caltech
)
,
Michele Vallisneri
(
- Caltech
)

- Phys.Rev.D 67 (2003) 024016,
- Phys.Rev.D 74 (2006) 029903 (erratum)
•
e-Print:
- gr-qc/0205122
•
DOI:
- 10.1103/PhysRevD.67.024016

Detecting gravitational waves from precessing binaries of spinning compact objects: Adiabatic limit

Alessandra Buonanno
(
- Paris, Inst. Astrophys. and
- Caltech
)
,
Yan-bei Chen
(
- Caltech
)
,
Michele Vallisneri
(
- Caltech, JPL and
- Caltech
)

- Phys.Rev.D 67 (2003) 104025,
- Phys.Rev.D 74 (2006) 029904 (erratum)
•
e-Print:
- gr-qc/0211087
•
DOI:
- 10.1103/PhysRevD.67.104025

Innermost circular orbit of binary black holes at the third postNewtonian approximation

Luc Blanchet
(
- Paris, Inst. Astrophys.
)

- Phys.Rev.D 65 (2002) 124009
•
e-Print:
- gr-qc/0112056
•
DOI:
- 10.1103/PhysRevD.65.124009

Coalescing binary neutron stars

Christopher S. Kochanek
(
- Harvard-Smithsonian Ctr. Astrophys.
)

- Astrophys.J. 398 (1992) 234
•
DOI:
- 10.1086/171851

Tidal interactions of inspiraling compact binaries

- Astrophys.J. 400 (1992) 175-180
•
DOI:
- 10.1086/171983

Radiation reaction and the selfforce for a point mass in general relativity

Steven L. Detweiler
(
- Florida U.
)

- Phys.Rev.Lett. 86 (2001) 1931-1934
•
e-Print:
- gr-qc/0011039
•
DOI:
- 10.1103/PhysRevLett.86.1931

Retarded coordinates based at a world line, and the motion of a small black hole in an external universe

Eric Poisson
(
- Guelph U. and
- Perimeter Inst. Theor. Phys.
)

- Phys.Rev.D 69 (2004) 084007
•
e-Print:
- gr-qc/0311026
•
DOI:
- 10.1103/PhysRevD.69.084007

An Approximate binary black hole metric

Kashif Alvi
(
- Caltech
)

- Phys.Rev.D 61 (2000) 124013
•
e-Print:
- gr-qc/9912113
•
DOI:
- 10.1103/PhysRevD.61.124013

Note on ingoing coordinates for binary black holes

Kashif Alvi
(
- Caltech
)

- Phys.Rev.D 67 (2003) 104006
•
e-Print:
- gr-qc/0302061
•
DOI:
- 10.1103/PhysRevD.67.104006

Post-Newtonian gravitational radiation and equations of motion via direct integration of the relaxed Einstein equations. III. Radiation reaction for binary systems with spinning bodies

Clifford M. Will
(
- Paris, Inst. Astrophys. and
- McDonnell Ctr. Space Sci.
)

- Phys.Rev.D 71 (2005) 084027
•
e-Print:
- gr-qc/0502039
•
DOI:
- 10.1103/PhysRevD.71.084027

Coalescing binary systems of compact objects to postNewtonian 5/2 order. 5. Spin effects

Lawrence E. Kidder
(
- Washington U., St. Louis
)

- Phys.Rev.D 52 (1995) 821-847
•
e-Print:
- gr-qc/9506022
•
DOI:
- 10.1103/PhysRevD.52.821

Gravitational waves from inspiraling compact binaries: The Quadrupole moment term

Eric Poisson
(
- Guelph U.
)

- Phys.Rev.D 57 (1998) 5287-5290
•
e-Print:
- gr-qc/9709032
•
DOI:
- 10.1103/PhysRevD.57.5287

Gravitational waves from inspiralling compact binaries with magnetic dipole moments

- Astrophys.J. 537 (2000) 327
•
e-Print:
- astro-ph/0001218
•
DOI:
- 10.1086/309004

Gravitational Radiation and the Motion of Two Point Masses

P.C. Peters
(
- Caltech
)

- Phys.Rev. 136 (1964) B1224-B1232
•
DOI:
- 10.1103/PhysRev.136.B1224

1-25 of 46
1
2
25 / page