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The detection of a stochastic background of low-frequency gravitational waves by pulsar-timing and astrometric surveys will enable tests of gravitational theories beyond general relativity.
1904
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1906
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1909
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1911
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John O’Hanlon, “Intermediate-range gravity - a generally covariant model,” Phys. Rev. Lett. 29
1972
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R. w. Hellings and G. s. Downs, “UPPER LIMITS ON THE ISOTROPIC GRAVITATIONAL RADIATION BACKGROUND FROM PULSAR TIMING ANALYSIS,” Astrophys. J. 265
1983
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P. Teyssandier and Ph. Tourrenc, “The Cauchy problem for the R+R**2 theories of gravity without torsion,” J. Math. Phys. 24
1983
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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. B105
1990
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Nick Kaiser and Andrew H. Jaffe, “Bending of light by gravity waves,” Astrophys. J. 484
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Takeshi Chiba, Tristan L. Smith, and Adrienne L. Erickcek, “Solar System constraints to general f(R) gravity,” Phys. Rev. D75
2007
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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
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2008
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2012
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G. Hobbs, “The Parkes Pulsar Timing Array,” Class. Quant. Grav. 30
2013
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R. N. Manchester et al. , “The Parkes Pulsar Timing Array Project,” Publ. Astron. Soc. Austral. 30
2013
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