Abstract
Many objects discovered by LIGO and Virgo are peculiar because they fall in a mass range which in the past was considered unpopulated by compact objects. Given the significance of the astrophysical implications, it is important to first understand how their masses are measured from gravitational-wave signals. How accurate is the measurement? Are there elements missing in our current model which may result in a bias? This chapter is dedicated to these questions. In particular, we will highlight several astrophysical factors which are not included in the standard model of GW sources but could result in a significant bias in the estimation of the mass. These factors include strong gravitational lensing, a relative motion of the source, a nearby massive object, and a gaseous background.
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References
Abbott BP, Abbott R, Abbott TD, Abernathy MR, Acernese F, Ackley K, Adams C, Adams T, Addesso P, Adhikari RX, et al (2016) Observation of gravitational waves from a binary black hole merger. Phys Rev Lett 116:061102
LIGO Scientific Collaboration and Virgo Collaboration (2019) Binary black hole population properties inferred from the first and second observing runs of advanced LIGO and advanced Virgo. Astrophys J Lett 882:L24
LIGO Scientific Collaboration and Virgo Collaboration (2020) GW190425: observation of a compact binary coalescence with total mass ∼3.4 m ⊙. Astrophys J 892:L3
L. S. Collaboration and V. Collaboration (2020) Gw190521: a binary black hole merger with a total mass of \(150{M}_{{\bigodot }}\). Phys Rev Lett 125:101102
Miller MC, Hamilton DP (2002) Four-body effects in globular cluster black hole coalescence. Astrophys J 576:894–898
Antonini F, Perets HB (2012) Secular evolution of compact binaries near massive black holes: gravitational Wave Sources and Other Exotica. Astrophys J 757:27
Chen X, Li S, Cao Z (2019) Mass-redshift degeneracy for the gravitational-wave sources in the vicinity of supermassive black holes. Mon Not R Astron Soc 485:L141–L145
Chen X, Xuan Z-Y, Peng P (2020) Fake massive black holes in the milli-hertz gravitational-wave band. Astrophys J 896:171
Marković D (1993) Possibility of determining cosmological parameters from measurements of gravitational waves emitted by coalescing, compact binaries. Phys Rev D 48:4738–4756
Wang Y, Stebbins A, Turner EL (1996) Gravitational lensing of gravitational waves from merging neutron star binaries. Phys Rev Lett 77:2875–2878
Nakamura TT (1998) Gravitational lensing of gravitational waves from inspiraling binaries by a point mass lens. Phys Rev Lett 80:1138–1141
Takahashi R, Nakamura T (2003) Wave effects in the gravitational lensing of gravitational waves from chirping binaries. Astrophys J 595:1039–1051
Schutz BF (1986) Determining the Hubble constant from gravitational wave observations. Nature 323:310
Peters PC (1964) Gravitational radiation and the motion of two point masses. Phys Rev 136:1224–1232
Sathyaprakash BS, Schutz BF (2009) Physics, astrophysics and cosmology with gravitational waves. Living Rev Relativ 12:2
Amaro-Seoane P, Audley H, Babak S, Baker J, Barausse E, Bender P, Berti E, Binetruy P, Born M, Bortoluzzi DEA (2017) Laser interferometer space antenna. ArXiv e-prints
Broadhurst T, Diego JM, Smoot GI (2018) Reinterpreting low frequency LIGO/Virgo events as magnified stellar-mass black holes at cosmological distances. arXiv e-prints, arXiv:1802.05273
Smith GP, Jauzac M, Veitch J, Farr WM, Massey R, Richard J (2018) What if LIGO’s gravitational wave detections are strongly lensed by massive galaxy clusters? Mon Not R Astron Soc 475:3823–3828
LIGO Scientific Collaboration and Virgo Collaboration (2019) GWTC-1: a gravitational-wave transient catalog of compact binary mergers observed by LIGO and Virgo during the first and second observing runs. Phys Rev X 9:031040
Laguna P, Larson SL, Spergel D, Yunes N (2010) Integrated Sachs-Wolfe effect for gravitational radiation. Astrophys J Lett 715:L12–L15
Torres-Orjuela A, Chen X, Cao Z, Amaro-Seoane P, Peng P (2019) Detecting the beaming effect of gravitational waves. Phys Rev D 100:063012
Abbott BP, Abbott R, Abbott TD, Abernathy MR, Acernese F, Ackley K, Adams C, Adams T, Addesso P, Adhikari RX, et al (2016) Astrophysical implications of the binary black-hole merger GW150914. Astrophys J Lett 818:L22
Meiron Y, Kocsis B, Loeb A (2017) Detecting triple systems with gravitational wave observations. Astrophys J 834:200
Inayoshi K, Tamanini N, Caprini C, Haiman Z (2017) Probing stellar binary black hole formation in galactic nuclei via the imprint of their center of mass acceleration on their gravitational wave signal. Phys Rev D 96:063014
Tamanini N, Klein A, Bonvin C, Barausse E, Caprini C (2020) Peculiar acceleration of stellar-origin black hole binaries: measurement and biases with LISA. Phys Rev D 101:063002
Robson T, Cornish NJ, Tamanini N, Toonen S (2018) Detecting hierarchical stellar systems with LISA. Phys Rev D 98:064012
Chen X, Shen Z (2019) Retrieving the true masses of gravitational wave sources. Proceedings 17(1):4
Caputo A, Sberna L, Toubiana A, Babak S, Barausse E, Marsat S, Pani P (2020) Gravitational-wave detection and parameter estimation for accreting black-hole binaries and their electromagnetic counterpart. Astrophys J 892:90
Hannuksela OA, Haris K, Ng KKY, Kumar S, Mehta AK, Keitel D, Li TGF, Ajith P (2019) Search for gravitational lensing signatures in LIGO-virgo binary black hole events. Astrophys J 874:L2
Torres-Orjuela A, Chen X, Amaro-Seoane P (2020) Phase shift of gravitational waves induced by aberration. Phys Rev D 101:083028
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Chen, X. (2022). Distortion of Gravitational-Wave Signals by Astrophysical Environments. In: Bambi, C., Katsanevas, S., Kokkotas, K.D. (eds) Handbook of Gravitational Wave Astronomy. Springer, Singapore. https://doi.org/10.1007/978-981-16-4306-4_39
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