The DOI matches its Crossref record; 131 of the 131 references it cites were found in a registry or an index.
Probing ultralight bosons with binary black holes
Open accessAbstract
We study the gravitational-wave (GW) signatures of clouds of ultralight bosons around black holes (BHs) in binary inspirals.These clouds, which are formed via superradiance instabilities for rapidly rotating BHs, produce distinct effects in the population of BH masses and spins, and a continuous monochromatic GW signal.We show that the presence of a binary companion greatly enriches the dynamical evolution of the system, most remarkably through the existence of resonant transitions between the growing and decaying modes of the cloud (analogous to Rabi oscillations in atomic physics).These resonances have rich phenomenological implications for current and future GW detectors.Notably, the amplitude of the GW signal from the clouds may be reduced, and in many cases terminated, much before the binary merger.The presence of a boson cloud can also be revealed in the GW signal from the binary through the imprint of finite-size effects, such as spin-induced multipole moments and tidal Love numbers.The time dependence of the cloud's energy density during the resonance leads to a sharp feature, or at least attenuation, in the contribution from the finitesize terms to the waveforms.The observation of these effects would constrain the properties of putative ultralight bosons through precision GW data, offering new probes of physics beyond the Standard Model.
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Observation of Gravitational Waves from a Binary Black Hole Merger
Abbott, B. P., Abbott, R., Abbott, T. D., Abernathy, M. R., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R. X., et al. (2016) · Physical Review Letters · doi:10.1103/physrevlett.116.061102 · Cited by 14,151
GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
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Multi-messenger Observations of a Binary Neutron Star Merger*
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Self-citationGW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
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GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2
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Self-citationQuantum gravity phenomenology at the dawn of the multi-messenger era—A review
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The spectra of gravitational atoms
Baumann, D., Chia, H. S., Stout, J., & Haar, L. T. (2019) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/12/006 · Cited by 194
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Metadata
- Authors
- Baumann, D., Chia, H. S., & Porto, R. A.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 2019-02-04
- Volume
- 99
- Issue
- 4
- ISSN
- 2470-0010 (ISSN-L)
- 2470-0029
- OpenAlex
- W2796939409
- Cited by
- 294
- References
- 131
- FWCI
- 16.68
- Type
- journal article
- Language
- en
- Open access
- bronze
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