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We discuss the theory of pulsar-timing and astrometry probes of a stochastic gravitational-wave background with a recently developed "total-angular-momentum" (TAM) formalism for cosmological perturbations.
D. M. Eardley, D. L. Lee and A. P. Lightman, “Gravitational-wave observations as a tool for testing relativistic gravity,” Phys. Rev. D 8
1973
Earlier work this paper cites.
M. V. Sazhin, “Opportunities for detecting ultralong gravitational waves,” Sov. Astron. 22
1978
Earlier work this paper cites.
S. L. Detweiler, “Pulsar timing measurements and the search for gravitational waves,” Astrophys. J. 234
1979
Earlier work this paper cites.
R. W. Hellings and G. S. Downs, “Upper Limits On The Isotropic Gravitational Radiation Background From Pulsar Timing Analysis,” Astrophys. J. 265
1983
Earlier work this paper cites.
R. S. Foster and D. C. Backer, “Constructing a pulsar timing array,” Astrophys. J. 361
1990
Earlier work this paper cites.
V. B. Braginsky, N. S. Kardashev, I. D. Novikov and A. G. Polnarev, “Propagation of electromagnetic radiation in a random field of gravitational waves and space radio interferometry,” Nuovo Cim. B 105
1990
Earlier work this paper cites.
M. Rajagopal and R. W. Romani, “Ultralow frequency gravitational radiation from massive black hole binaries,” Astrophys. J. 446
1995
Earlier work this paper cites.
N. Kaiser and A. H. Jaffe, “Bending of light by gravity waves,” Astrophys. J. 484
1997
Earlier work this paper cites.
M. Kamionkowski, A. Kosowsky and A. Stebbins, “Statistics of cosmic microwave background polarization,” Phys. Rev. D 55
1997
Earlier work this paper cites.
M. Maggiore, “Gravitational wave experiments and early universe cosmology,” Phys. Rept. 331
2000
Earlier work this paper cites.
A. H. Jaffe and D. C. Backer, “Gravitational waves probe the coalescence rate of massive black hole binaries,” Astrophys. J. 583
2003
Earlier work this paper cites.
A. Hajian and T. Souradeep, “Measuring statistical isotropy of the CMB anisotropy,” Astrophys. J. 597
2003
Earlier work this paper cites.
N. L. Zakamska and S. Tremaine, “Constraints on the acceleration of the solar system from high-precision timing,” Astron. J. 130
2005
Earlier work this paper cites.
M. Enoki and M. Nagashima, “The Effect of Orbital Eccentricity on Gravitational Wave Background Radiation from Supermassive Black Hole Binaries,” Prog. Theor. Phys. 117
2007
Earlier work this paper cites.
K. J. Lee, F. A. Jenet, and R. H. Price, “Pulsar timing as a probe of non-einsteinian polarizations of gravitational waves,” Astrophys. J. 685
2008
Earlier work this paper cites.
2008
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2009
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2009
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2011
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2012
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2012
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2012
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2012
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2012
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D. Jeong and M. Kamionkowski, “Clustering Fossils from the Early Universe,” Phys. Rev. Lett. 108
2012
Cited alongside, same era.
G. Hobbs, “The Parkes Pulsar Timing Array,” Class. Quant. Grav. 30
2013
Cited alongside, same era.
2013
Cited alongside, same era.
2013
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2013
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2013
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2017
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2017
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2017
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2017
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2017
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2018
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2018
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2018
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2018
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M. Kamionkowski, “Circular polarization in a spherical basis,” Phys. Rev. D 97
2018
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M. Maggiore, Gravitational waves, volume II: astrophysics and cosmology
2018
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2018
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