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We use the gravitational wave (GW) events GW170817 and GW190521, together with their proposed electromagnetic counterparts, to constrain cosmological parameters and theories of gravity beyond General Relativity (GR).
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C. Deffayet and K. Menou, Probing Gravity with Spacetime Sirens , Astrophys. J. Lett. 668
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W.L. Freedman, Correction: Cosmology at a crossroads , Nature Astronomy 1
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J.M. Ezquiaga and M. Zumalacárregui, Dark Energy in light of Multi-Messenger Gravitational-Wave astronomy , Frontiers in Astronomy and Space Sciences 5
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M. Tse et al., Quantum-Enhanced Advanced LIGO Detectors in the Era of Gravitational-Wave Astronomy , Phys. Rev. Lett. 123
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R. Abbott, T.D. Abbott, S. Abraham, F. Acernese, K. Ackley, C. Adams et al., GW190521: A Binary Black Hole Merger with a Total Mass of 150 M ⊙
2020
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R. Abbott, T.D. Abbott, S. Abraham, F. Acernese, K. Ackley, C. Adams et al., Properties and astrophysical implications of the 150 m ⊙ \odot binary black hole merger GW190521 , The Astrophysical Journal 900
2020
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