The unresolved stochastic background from compact binary mergers detectable by next-generation ground-based gravitational-wave observatories

Nicholas Farrow, Xing-Jiang Zhu, and Eric Thrane, “The mass distribution of Galactic double neutron stars,” Astrophys. J. 876

Original

1902

Earlier work this paper cites.

Vassiliki Kalogera et al. , “Deeper, Wider, Sharper: Next-Generation Ground-Based Gravitational-Wave Observations of Binary Black Holes,” (2019), arXiv:1903.09220 [astro-ph.HE]

Original

1903

Earlier work this paper cites.

B. P. Abbott et al. (LIGO Scientific, Virgo), “Search for the isotropic stochastic background using data from Advanced LIGO’s second observing run,” Phys. Rev. D 100

Original

1903

Earlier work this paper cites.

Paz Beniamini and Tsvi Piran, “The Gravitational waves merger time distribution of binary neutron star systems,” Mon. Not. Roy. Astron. Soc. 487

Original

1903

Earlier work this paper cites.

Maya Fishbach and Daniel E. Holz, “Picky Partners: The Pairing of Component Masses in Binary Black Hole Mergers,” Astrophys. J. Lett. 891

Original

1905

Earlier work this paper cites.

Daniel G. Figueroa and Erwin H. Tanin, “Ability of LIGO and LISA to probe the equation of state of the early Universe,” JCAP 08

Original

1905

Earlier work this paper cites.

Maya Fishbach, Will M. Farr, and Daniel E. Holz, “The Most Massive Binary Black Hole Detections and the Identification of Population Outliers,” Astrophys. J. Lett. 891

Original

1911

Earlier work this paper cites.

Michele Maggiore et al. , “Science Case for the Einstein Telescope,” JCAP 03

Original

1912

Earlier work this paper cites.

Tsvi Piran, “The Implications of the Compton (GRO) Observations for Cosmological Gamma-Ray Bursts,” Astrophys. J. Lett. 389

1992

Earlier work this paper cites.

Valeria Ferrari, Sabino Matarrese, and Raffaella Schneider, “Stochastic background of gravitational waves generated by a cosmological population of young, rapidly rotating neutron stars,” Mon. Not. Roy. Astron. Soc. 303

1999

Earlier work this paper cites.

David W. Hogg, “Distance measures in cosmology,” (1999), arXiv:astro-ph/9905116

1999

Earlier work this paper cites.

Bruce Allen and Joseph D. Romano, “Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities,” Phys. Rev. D 59

1999

Earlier work this paper cites.

E. S. Phinney, “A Practical theorem on gravitational wave backgrounds,” (2001), arXiv:astro-ph/0108028

2001

Earlier work this paper cites.

Krzysztof Belczynski and Vassiliki Kalogera, “A New formation channel for double neutron stars without recycling: Implications for gravitational wave detection,” Astrophys. J. Lett. 550

2001

Earlier work this paper cites.

B. P. Abbott et al. (LIGO Scientific, Virgo), “GW190425: Observation of a Compact Binary Coalescence with Total Mass ∼ 3.4 ​ M ⊙ \sim 3.4M_{\odot} ,” Astrophys. J. Lett. 892

Original

2001

Earlier work this paper cites.

Isobel M. Romero-Shaw, Nicholas Farrow, Simon Stevenson, Eric Thrane, and Xing-Jiang Zhu, “On the origin of GW190425,” Mon. Not. Roy. Astron. Soc. 496

Original

2001

Earlier work this paper cites.

Surabhi Sachdev, Tania Regimbau, and B. S. Sathyaprakash, “Subtracting compact binary foreground sources to reveal primordial gravitational-wave backgrounds,” Phys. Rev. D 102

Original

2002

Earlier work this paper cites.

Thomas Callister, Maya Fishbach, Daniel Holz, and Will Farr, “Shouts and Murmurs: Combining Individual Gravitational-Wave Sources with the Stochastic Background to Measure the History of Binary Black Hole Mergers,” Astrophys. J. Lett. 896

Original

2003

Earlier work this paper cites.

Mohammadtaher Safarzadeh, Sylvia Biscoveanu, and Abraham Loeb, “Constraining the delay time distribution of compact binary objects from the stochastic gravitational wave background searches,” Astrophys. J. 901

Original

2004

Earlier work this paper cites.

Rory J. E. Smith, Colm Talbot, Francisco Hernandez Vivanco, and Eric Thrane, “Inferring the population properties of binary black holes from unresolved gravitational waves,” Mon. Not. Roy. Astron. Soc. 496

Original

2004

Earlier work this paper cites.

Alessandra Buonanno, Gunter Sigl, Georg G. Raffelt, Hans-Thomas Janka, and Ewald Muller, “Stochastic gravitational wave background from cosmological supernovae,” Phys. Rev. D 72

2005

Earlier work this paper cites.

Ashish Sharma and Jan Harms, “Searching for cosmological gravitational-wave backgrounds with third-generation detectors in the presence of an astrophysical foreground,” Phys. Rev. D 102

Original

2006

Earlier work this paper cites.

Krzysztof Belczynski, Rosalba Perna, Tomasz Bulik, Vassiliki Kalogera, Natalia Ivanova, and Donald Q. Lamb, “A study of compact object mergers as short gamma-ray burst progenitors,” Astrophys. J. 648

2006

Earlier work this paper cites.

Maya Fishbach, Reed Essick, and Daniel E. Holz, “Does Matter Matter? Using the mass distribution to distinguish neutron stars and black holes,” Astrophys. J. Lett. 899

Original

2006

Earlier work this paper cites.

Sharan Banagiri, Vuk Mandic, Claudia Scarlata, and Kate Z. Yang, “Measuring angular N-point correlations of binary black hole merger gravitational-wave events with hierarchical Bayesian inference,” Phys. Rev. D 102

Original

2006

Earlier work this paper cites.

Edo Berger et al. , “A New Population of High Redshift Short-Duration Gamma-Ray Bursts,” Astrophys. J. 664

2007

Earlier work this paper cites.

Richard Easther, John T. Giblin, Jr., and Eugene A. Lim, “Gravitational Wave Production At The End Of Inflation,” Phys. Rev. Lett. 99

2007

Earlier work this paper cites.

T. Regimbau and V. Mandic, “Astrophysical Sources of Stochastic Gravitational-Wave Background,” Class. Quant. Grav. 25

Original

2008

Earlier work this paper cites.

C. Périgois, C. Belczynski, T. Bulik, and T. Regimbau, “StarTrack predictions of the stochastic gravitational-wave background from compact binary mergers,” Phys. Rev. D 103

Original

2008

Earlier work this paper cites.

Sylvia Biscoveanu, Colm Talbot, Eric Thrane, and Rory Smith, “Measuring the primordial gravitational-wave background in the presence of astrophysical foregrounds,” Phys. Rev. Lett. 125

Original

2009

Earlier work this paper cites.

R. Abbott et al. (LIGO Scientific, Virgo), “GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run,” Phys. Rev. X 11

Original

2010

Earlier work this paper cites.

M. Punturo et al. , “The Einstein Telescope: A third-generation gravitational wave observatory,” Class. Quant. Grav. 27

2010

Cited alongside, same era.

Ssohrab Borhanian, “GWBENCH: a novel Fisher information package for gravitational-wave benchmarking,” Class. Quant. Grav. 38

Original

2010

Cited alongside, same era.

Jose R. Espinosa, Thomas Konstandin, Jose M. No, and Geraldine Servant, “Energy Budget of Cosmological First-order Phase Transitions,” JCAP 06

Original

2010

Cited alongside, same era.

Tania Regimbau, “The astrophysical gravitational wave stochastic background,” Res. Astron. Astrophys. 11

Original

2011

Cited alongside, same era.

Katarina Martinovic, Patrick M. Meyers, Mairi Sakellariadou, and Nelson Christensen, “Simultaneous estimation of astrophysical and cosmological stochastic gravitational-wave backgrounds with terrestrial detectors,” Phys. Rev. D 103

Chiara Caprini and Daniel G. Figueroa, “Cosmological Backgrounds of Gravitational Waves,” Class. Quant. Grav. 35

Original

2018

Later among the works it cites.

Maya Fishbach, Daniel E. Holz, and Will M. Farr, “Does the Black Hole Merger Rate Evolve with Redshift?” Astrophys. J. Lett. 863

Original

2018

Later among the works it cites.

Rory Smith and Eric Thrane, “Optimal Search for an Astrophysical Gravitational-Wave Background,” Phys. Rev. X 8

Original

2018

Later among the works it cites.

Nelson Christensen, “Stochastic Gravitational Wave Backgrounds,” Rept. Prog. Phys. 82

Original

2019

Later among the works it cites.

Alexander C. Jenkins, Richard O’Shaughnessy, Mairi Sakellariadou, and Daniel Wysocki, “Anisotropies in the astrophysical gravitational-wave background: The impact of black hole distributions,” Phys. Rev. Lett. 122