001     604086
005     20241103101401.0
024 7 _ |a arXiv:2403.02415
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024 7 _ |a 10.3204/PUBDB-2024-00990
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037 _ _ |a PUBDB-2024-00990
041 _ _ |a English
088 _ _ |a DESY-24-030
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088 _ _ |a arXiv:2403.02415
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100 1 _ |a Boskovic, Mateja
|0 P:(DE-H253)PIP1108088
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245 _ _ |a Signatures of ultralight bosons in the orbital eccentricity of binary black holes
260 _ _ |c 2024
336 7 _ |a Preprint
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336 7 _ |a Electronic Article
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336 7 _ |a preprint
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336 7 _ |a ARTICLE
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336 7 _ |a Output Types/Working Paper
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500 _ _ |a 5 pages + 9 pages appendices and references, 8 figures
520 _ _ |a We show that the existence of clouds of ultralight particles surrounding black holes during their cosmological history as members of a binary system can leave a measurable imprint on the distribution of masses and orbital eccentricities observable with future gravitational-wave detectors. Notably, we find that for nonprecessing binaries with chirp masses ${\cal M} \lesssim 10 M_\odot$, formed by and large in isolation, greater-than-expected values of the eccentricity, i.e. $e\gtrsim 10^{-2}$ at gravitational-wave frequencies $f_{\rm GW} \simeq 10^{-2}$Hz, would provide tantalizing evidence for a new particle of mass between $[0.5,2.5] \times 10^{-12}\,$eV in nature. The predicted evolution of the eccentricity can also drastically affect the in-band phase evolution and peak frequency. These results constitute unique signatures of boson clouds of ultralight particles in the dynamics of binary black holes, which will be readily accessible with the Laser Interferometer Space Antenna, as well as future mid-band and Deci-hertz detectors.
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650 _ 7 |a black hole, binary
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650 _ 7 |a gravitational radiation, frequency
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650 _ 7 |a new particle, mass
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650 _ 7 |a boson, signature
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650 _ 7 |a cloud
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650 _ 7 |a gravitational radiation detector
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650 _ 7 |a LISA
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700 1 _ |a Koschnitzke, Matthias
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700 1 _ |a Porto Pereira, Rafael Alejandro
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910 1 _ |a Deutsches Elektronen-Synchrotron
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