Built on

T. W. B. Kibble, “Topology of cosmic domains and strings,” J. Phys. A 9
1976
Earlier work this paper cites.
A. A. Starobinsky, “Spectrum of relic gravitational radiation and the early state of the universe,” Zh. Eksp. Teor. Fiz., Pis’ma Red 30
1979
Earlier work this paper cites.
R. R. Caldwell and B. Allen, “Cosmological constraints on cosmic-string gravitational radiation,” Phys. Rev. D 45
1992
Earlier work this paper cites.
A. Kosowsky, M. S. Turner, and R. Watkins, “Gravitational waves from first-order cosmological phase transitions,” Phys. Rev. Lett. 69
1992
Earlier work this paper cites.
N. Christensen, “Measuring the stochastic gravitational-radiation background with laser-interferometric antennas,” Phys. Rev. D 46
1992
Earlier work this paper cites.
B. Allen and J. D. Romano, “Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities,” Phys. Rev. D 59
1999
Earlier work this paper cites.
M. Maggiore, “Gravitational wave experiments and early universe cosmology,” Phys. Rep. 331
2000
Earlier work this paper cites.
E. S. Phinney, “A practical theorem on gravitational wave backgrounds,” ArXiv e-prints (2001), arXiv:astro-ph/0108028
2001
Earlier work this paper cites.
P. Ajith, S. Babak, Y. Chen, M. Hewitson, B. Krishnan, A. M. Sintes, J. T. Whelan, B. Brügmann, P. Diener, N. Dorband, et al. , “Template bank for gravitational waveforms from coalescing binary black holes: Nonspinning binaries,” Phys. Rev. D 77
Original
2008
Earlier work this paper cites.
J. Abadie et al. (LIGO Scientific Collaboration and Virgo Collaboration), “TOPICAL REVIEW: Predictions for the rates of compact binary coalescences observable by ground-based gravitational-wave detectors,” Classical and Quantum Gravity 27
Original
2010
Earlier work this paper cites.
M. Punturo, M. Abernathy, F. Acernese, B. Allen, N. Andersson, K. Arun, F. Barone, B. Barr, M. Barsuglia, and M. Beker, “The einstein telescope: a third-generation gravitational wave observatory,” Classical and Quantum Gravity 27
2010
Earlier work this paper cites.

Similar

X.-J. Zhu, E. Howell, T. Regimbau, D. Blair, and Z.-H. Zhu, “Stochastic gravitational wave background from coalescing binary black holes,” Astrophys. J. 739
Original
2011
Cited alongside, same era.
P. A. Rosado, “Gravitational wave background from binary systems,” Phys. Rev. D 84
Original
2011
Cited alongside, same era.
S. Marassi, R. Schneider, G. Corvino, V. Ferrari, and S. P. Zwart, “Imprint of the merger and ring-down on the gravitational wave background from black hole binaries coalescence,” Phys. Rev. D 84
Original
2011
Cited alongside, same era.
C. Wu, V. Mandic, and T. Regimbau, “Accessibility of the gravitational-wave background due to binary coalescences to second and third generation gravitational-wave detectors,” Phys. Rev. D 85
Original
2012
Cited alongside, same era.

Then

E. Thrane, “Measuring the non-gaussian stochastic gravitational-wave background: a method for realistic interferometer data,” Phys. Rev. D 87
Original
2013
Later among the works it cites.
J. T. Giblin, Jr. and E. Thrane, “The detectability of cosmological gravitational-wave backgrounds: a rule of thumb,” Phys. Rev. D 90
Original
2014
Later among the works it cites.
L. Martellini and T. Regimbau, “Semiparametric approach to the detection of non-gaussian gravitational wave stochastic backgrounds,” Phys. Rev. D 89
Original
2014
Later among the works it cites.
P. Madau and M. Dickinson, “Cosmic star-formation history,” Annu. Rev. Astron. Astrophys. 52
Original
2014
Later among the works it cites.
J. Aasi et al. (LIGO Scientific Collaboration), “Advanced LIGO,” Classical and Quantum Gravity 32

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2016

Limits of Astrophysics with Gravitational-Wave Backgrounds

Callister, Thomas, Sammut, Letizia, Qiu, Shi et al.

Understand

The recent Advanced LIGO detection of gravitational waves from the binary black hole GW150914 suggests there exists a large population of merging binary black holes in the Universe.

Although most are too distant to be individually resolved by advanced detectors, the superposition of gravitational waves from many unresolvable binaries is expected to create an astrophysical stochastic background.
Recent results from the LIGO and Virgo collaborations show that this astrophysical background is within reach of Advanced LIGO.
In principle, the binary black hole background encodes interesting astrophysical properties, such as the mass distribution and redshift distribution of distant binaries.

Built on

T. W. B. Kibble, “Topology of cosmic domains and strings,” J. Phys. A 9
1976
Earlier work this paper cites.
A. A. Starobinsky, “Spectrum of relic gravitational radiation and the early state of the universe,” Zh. Eksp. Teor. Fiz., Pis’ma Red 30
1979
Earlier work this paper cites.
R. R. Caldwell and B. Allen, “Cosmological constraints on cosmic-string gravitational radiation,” Phys. Rev. D 45
1992
Earlier work this paper cites.
A. Kosowsky, M. S. Turner, and R. Watkins, “Gravitational waves from first-order cosmological phase transitions,” Phys. Rev. Lett. 69
1992
Earlier work this paper cites.
N. Christensen, “Measuring the stochastic gravitational-radiation background with laser-interferometric antennas,” Phys. Rev. D 46
1992
Earlier work this paper cites.
B. Allen and J. D. Romano, “Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities,” Phys. Rev. D 59
1999
Earlier work this paper cites.
M. Maggiore, “Gravitational wave experiments and early universe cosmology,” Phys. Rep. 331
2000
Earlier work this paper cites.
E. S. Phinney, “A practical theorem on gravitational wave backgrounds,” ArXiv e-prints (2001), arXiv:astro-ph/0108028
2001
Earlier work this paper cites.
P. Ajith, S. Babak, Y. Chen, M. Hewitson, B. Krishnan, A. M. Sintes, J. T. Whelan, B. Brügmann, P. Diener, N. Dorband, et al. , “Template bank for gravitational waveforms from coalescing binary black holes: Nonspinning binaries,” Phys. Rev. D 77
Original
2008
Earlier work this paper cites.
J. Abadie et al. (LIGO Scientific Collaboration and Virgo Collaboration), “TOPICAL REVIEW: Predictions for the rates of compact binary coalescences observable by ground-based gravitational-wave detectors,” Classical and Quantum Gravity 27
Original
2010
Earlier work this paper cites.
M. Punturo, M. Abernathy, F. Acernese, B. Allen, N. Andersson, K. Arun, F. Barone, B. Barr, M. Barsuglia, and M. Beker, “The einstein telescope: a third-generation gravitational wave observatory,” Classical and Quantum Gravity 27
2010
Earlier work this paper cites.

Similar

X.-J. Zhu, E. Howell, T. Regimbau, D. Blair, and Z.-H. Zhu, “Stochastic gravitational wave background from coalescing binary black holes,” Astrophys. J. 739
Original
2011
Cited alongside, same era.
P. A. Rosado, “Gravitational wave background from binary systems,” Phys. Rev. D 84
Original
2011
Cited alongside, same era.
S. Marassi, R. Schneider, G. Corvino, V. Ferrari, and S. P. Zwart, “Imprint of the merger and ring-down on the gravitational wave background from black hole binaries coalescence,” Phys. Rev. D 84
Original
2011
Cited alongside, same era.
C. Wu, V. Mandic, and T. Regimbau, “Accessibility of the gravitational-wave background due to binary coalescences to second and third generation gravitational-wave detectors,” Phys. Rev. D 85
Original
2012
Cited alongside, same era.

Then

E. Thrane, “Measuring the non-gaussian stochastic gravitational-wave background: a method for realistic interferometer data,” Phys. Rev. D 87
Original
2013
Later among the works it cites.
J. T. Giblin, Jr. and E. Thrane, “The detectability of cosmological gravitational-wave backgrounds: a rule of thumb,” Phys. Rev. D 90
Original
2014
Later among the works it cites.
L. Martellini and T. Regimbau, “Semiparametric approach to the detection of non-gaussian gravitational wave stochastic backgrounds,” Phys. Rev. D 89
Original
2014
Later among the works it cites.
P. Madau and M. Dickinson, “Cosmic star-formation history,” Annu. Rev. Astron. Astrophys. 52
Original
2014
Later among the works it cites.
J. Aasi et al. (LIGO Scientific Collaboration), “Advanced LIGO,” Classical and Quantum Gravity 32

Beyond the bibliography

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

Open on alphaXiv

alphaXiv is searching for related work…

M. Dominik, K. Belczynski, C. Fryer, D. E. Holz, E. Berti, T. Bulik, I. Mandel, and R. O’Shaughnessy, “Double compact objects I. the significance of the common envelope on merger rates,” Astrophys. J. 759

Original

2012

Cited alongside, same era.

V. Mandic, E. Thrane, S. Giampanis, and T. Regimbau, “Parameter estimation in searches for the stochastic gravitational-wave background,” Phys. Rev. Lett. 109

Original

2012

Cited alongside, same era.

B Sathyaprakash, M. Abernathy, F. Acernese, P. Ajith, B. Allen, P. Amaro-Seoane, N. Andersson, S. Aoudia, K. Arun, P. Astone, et al. , “Scientific Objectives of Einstein Telescope,” Classical and Quantum Gravity 30

Original

2012

Cited alongside, same era.

C.-J. Wu, V. Mandic, and T. Regimbau, “Accessibility of the stochastic gravitational wave background from magnetars to the interferometric gravitational wave detectors,” Phys. Rev. D 87

2013

Cited alongside, same era.

X.-J. Zhu, E. J. Howell, D. G. Blair, and Z.-H. Zhu, “On the gravitational wave background from compact binary coalescences in the band of ground-based interferometers,” Mon. Not. R. Astron. Soc. 431

Original

2013

Cited alongside, same era.

E. Thrane and J. D. Romano, “Sensitivity curves for searches for gravitational-wave backgrounds,” Phys. Rev. D 88

Original

2013

Cited alongside, same era.

M. D. Kistler, H. Yuksel, and A. M. Hopkins, “The cosmic star formation rate from the faintest galaxies in the unobservable universe,” ArXiv e-prints (2013) , arXiv:1305.1630

Original