Built on

E. Poisson and C. M. Will, Phys.Rev. D52
1995
Earlier work this paper cites.
S. Babak, R. Balasubramanian, D. Churches, T. Cokelaer, and B. S. Sathyaprakash, Classical and Quantum Gravity 23
2006
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P. Ajith, S. Babak, Y. Chen, M. Hewitson, B. Krishnan, et al. , Phys.Rev. D77
Original
2008
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P. Ajith, Class.Quant.Grav. 25
Original
2008
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L. Lindblom, B. Owen, and D. Brown, Physical Review D 78
2008
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M. Vallisneri, Physical Review D 77
2008
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M. Hannam, Class. Quant. Grav. 26
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2009
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F. Feroz, M. P. Hobson, and M. Bridges, Monthly Notices of the Royal Astronomical Society 398
Original
2009
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B. Abbott et al. (LIGO Scientific), Rept. Prog. Phys. 72
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2009
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D. Shoemaker (the Advanced LIGO Team), “Advanced LIGO Reference Design,” (2009), [LIGO-M060056]
2009
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Similar

The LIGO Scientific Collaboration, Advanced LIGO Anticipated Sensitivity Curves , Tech. Rep. LIGO-T0900288-v3 (LIGO Project, 2009)
2009
Cited alongside, same era.
M. Boyle, D. A. Brown, and L. Pekowsky, Class.Quant.Grav. 26
Original
2009
Cited alongside, same era.
A. Buonanno, B. Iyer, E. Ochsner, Y. Pan, and B. Sathyaprakash, Phys.Rev. D80
Original
2009
Cited alongside, same era.
J. Abadie et al. (LIGO Scientific), Class. Quant. Grav. 27
Original
2010
Cited alongside, same era.
L. Santamaria, F. Ohme, P. Ajith, B. Bruegmann, N. Dorband, et al. , Phys.Rev. D82
Original
2010
Cited alongside, same era.

Then

J. Abadie et al. (LIGO Scientific Collaboration and Virgo Collaboration), Phys. Rev. D 83
Original
2011
Later among the works it cites.
P. Ajith, Phys.Rev. D84
Original
2011
Later among the works it cites.
M. Dominik, K. Belczynski, C. Fryer, D. Holz, E. Berti, T. Bulik, I. Mandel, and R. O’Shaughnessy, arXiv.org astro-ph.HE
2012
Closest in time.
F. Ohme, Class.Quant.Grav. 29
Original
2012
Closest in time.
P. Ajith, M. Boyle, D. A. Brown, B. Brugmann, L. T. Buchman, et al. , Class.Quant.Grav. 29
Original
2012
Closest in time.

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2012

Degeneracy between mass and spin in black-hole-binary waveforms

Baird, Emily, Fairhurst, Stephen, Hannam, Mark et al.

Understand

We explore the degeneracy between mass and spin in gravitational waveforms emitted by black-hole binary coalescences.

We focus on spin-aligned waveforms and obtain our results using phenomenological models that were tuned to numerical-relativity simulations.
A degeneracy is known for low-mass binaries (particularly neutron-star binaries), where gravitational-wave detectors are sensitive to only the inspiral phase, and the waveform can be modelled by post-Newtonian theory.
Here, we consider black-hole binaries, where detectors will also be sensitive to the merger and ringdown, and demonstrate that the degeneracy persists across a broad mass range.

Built on

E. Poisson and C. M. Will, Phys.Rev. D52
1995
Earlier work this paper cites.
S. Babak, R. Balasubramanian, D. Churches, T. Cokelaer, and B. S. Sathyaprakash, Classical and Quantum Gravity 23
2006
Earlier work this paper cites.
P. Ajith, S. Babak, Y. Chen, M. Hewitson, B. Krishnan, et al. , Phys.Rev. D77
Original
2008
Earlier work this paper cites.
P. Ajith, Class.Quant.Grav. 25
Original
2008
Earlier work this paper cites.
L. Lindblom, B. Owen, and D. Brown, Physical Review D 78
2008
Earlier work this paper cites.
M. Vallisneri, Physical Review D 77
2008
Earlier work this paper cites.
M. Hannam, Class. Quant. Grav. 26
Original
2009
Earlier work this paper cites.
F. Feroz, M. P. Hobson, and M. Bridges, Monthly Notices of the Royal Astronomical Society 398
Original
2009
Earlier work this paper cites.
B. Abbott et al. (LIGO Scientific), Rept. Prog. Phys. 72
Original
2009
Earlier work this paper cites.
D. Shoemaker (the Advanced LIGO Team), “Advanced LIGO Reference Design,” (2009), [LIGO-M060056]
2009
Earlier work this paper cites.

Similar

The LIGO Scientific Collaboration, Advanced LIGO Anticipated Sensitivity Curves , Tech. Rep. LIGO-T0900288-v3 (LIGO Project, 2009)
2009
Cited alongside, same era.
M. Boyle, D. A. Brown, and L. Pekowsky, Class.Quant.Grav. 26
Original
2009
Cited alongside, same era.
A. Buonanno, B. Iyer, E. Ochsner, Y. Pan, and B. Sathyaprakash, Phys.Rev. D80
Original
2009
Cited alongside, same era.
J. Abadie et al. (LIGO Scientific), Class. Quant. Grav. 27
Original
2010
Cited alongside, same era.
L. Santamaria, F. Ohme, P. Ajith, B. Bruegmann, N. Dorband, et al. , Phys.Rev. D82
Original
2010
Cited alongside, same era.

Then

J. Abadie et al. (LIGO Scientific Collaboration and Virgo Collaboration), Phys. Rev. D 83
Original
2011
Later among the works it cites.
P. Ajith, Phys.Rev. D84
Original
2011
Later among the works it cites.
M. Dominik, K. Belczynski, C. Fryer, D. Holz, E. Berti, T. Bulik, I. Mandel, and R. O’Shaughnessy, arXiv.org astro-ph.HE
2012
Closest in time.
F. Ohme, Class.Quant.Grav. 29
Original
2012
Closest in time.
P. Ajith, M. Boyle, D. A. Brown, B. Brugmann, L. T. Buchman, et al. , Class.Quant.Grav. 29
Original
2012
Closest in time.

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

Y. Pan, A. Buonanno, L. T. Buchman, T. Chu, L. E. Kidder, et al. , Phys.Rev. D81

Original

2010

Cited alongside, same era.

J. Veitch and A. Vecchio, Phys. Rev. D 81

Original

2010

Cited alongside, same era.

G. M. Harry and the LIGO Scientific Collaboration, Class. Quant. Grav. 27

2010

Cited alongside, same era.

Shoemaker, David and Losurdo, Giovanni, Possible Scenarios for Commissioning and Early Observing with the Second Generation Detectors , Tech. Rep. LIGO-G10001760-v7 (LIGO Project, 2010)

2010

Cited alongside, same era.

P. Ajith, M. Hannam, S. Husa, Y. Chen, B. Bruegmann, et al. , Phys.Rev.Lett. 106

Original

2011

Cited alongside, same era.

C. Cutler and E. E. Flanagan, Phys.Rev. D49

Cited in the paper.

M. van der Sluys et al. , Classical and Quantum Gravity 25

Original

Cited in the paper.

P. Schmidt, M. Hannam, and S. Husa, (2012), arXiv:1207.3088 [gr-qc]