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| 001 | 616773 | ||
| 005 | 20250715170719.0 | ||
| 024 | 7 | _ | |a 10.1103/PhysRevLett.133.121401 |2 doi |
| 024 | 7 | _ | |a Boskovic:2024fga |2 INSPIRETeX |
| 024 | 7 | _ | |a inspire:2764914 |2 inspire |
| 024 | 7 | _ | |a 0031-9007 |2 ISSN |
| 024 | 7 | _ | |a 1092-0145 |2 ISSN |
| 024 | 7 | _ | |a 1079-7114 |2 ISSN |
| 024 | 7 | _ | |a arXiv:2403.02415 |2 arXiv |
| 024 | 7 | _ | |a 10.3204/PUBDB-2024-06527 |2 datacite_doi |
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| 037 | _ | _ | |a PUBDB-2024-06527 |
| 041 | _ | _ | |a English |
| 082 | _ | _ | |a 530 |
| 088 | _ | _ | |a arXiv:2403.02415 |2 arXiv |
| 088 | _ | _ | |a DESY-24-030 |2 DESY |
| 100 | 1 | _ | |a Bošković, Mateja |0 P:(DE-H253)PIP1108088 |b 0 |e Corresponding author |u desy |
| 245 | _ | _ | |a Signatures of Ultralight Bosons in the Orbital Eccentricity of Binary Black Holes |
| 260 | _ | _ | |a College Park, Md. |c 2024 |b APS |
| 336 | 7 | _ | |a article |2 DRIVER |
| 336 | 7 | _ | |a Output Types/Journal article |2 DataCite |
| 336 | 7 | _ | |a Journal Article |b journal |m journal |0 PUB:(DE-HGF)16 |s 1730282036_76827 |2 PUB:(DE-HGF) |
| 336 | 7 | _ | |a ARTICLE |2 BibTeX |
| 336 | 7 | _ | |a JOURNAL_ARTICLE |2 ORCID |
| 336 | 7 | _ | |a Journal Article |0 0 |2 EndNote |
| 500 | _ | _ | |a Phys.Rev.Lett. 133 (2024) 12, 121401. v2: 5 pages + 11 pages appendices and references, 11 figures; few typos corrected; added two sections to the appendices; published in PRL |
| 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 M≲10M⊙, formed exclusively in isolation, larger-than-expected values of the eccentricity, i.e., e≳10-2 at gravitational-wave frequencies fGW≃10-2 Hz, would provide tantalizing evidence for a new particle of mass between [0.5,2.5]×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 midband and decihertz detectors. |
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| 536 | _ | _ | |a LHCtoLISA - Precision Gravity: From the LHC to LISA (817791) |0 G:(EU-Grant)817791 |c 817791 |f ERC-2018-COG |x 2 |
| 542 | _ | _ | |i 2024-09-16 |2 Crossref |u https://link.aps.org/licenses/aps-default-license |
| 588 | _ | _ | |a Dataset connected to CrossRef, INSPIRE, Journals: bib-pubdb1.desy.de |
| 650 | _ | 7 | |a black hole: binary |2 INSPIRE |
| 650 | _ | 7 | |a gravitational radiation: frequency |2 INSPIRE |
| 650 | _ | 7 | |a new particle: mass |2 INSPIRE |
| 650 | _ | 7 | |a boson: signature |2 INSPIRE |
| 650 | _ | 7 | |a cloud |2 INSPIRE |
| 650 | _ | 7 | |a gravitational radiation detector |2 INSPIRE |
| 650 | _ | 7 | |a LISA |2 INSPIRE |
| 650 | _ | 7 | |a history |2 INSPIRE |
| 650 | _ | 7 | |a binary: orbit |2 INSPIRE |
| 693 | _ | _ | |0 EXP:(DE-MLZ)NOSPEC-20140101 |5 EXP:(DE-MLZ)NOSPEC-20140101 |e No specific instrument |x 0 |
| 700 | 1 | _ | |a Koschnitzke, Matthias |0 P:(DE-H253)PIP1086564 |b 1 |e Corresponding author |
| 700 | 1 | _ | |a Porto Pereira, Rafael Alejandro |0 P:(DE-H253)PIP1020780 |b 2 |e Corresponding author |u desy |
| 773 | 1 | 8 | |a 10.1103/physrevlett.133.121401 |b American Physical Society (APS) |d 2024-09-16 |n 12 |p 121401 |3 journal-article |2 Crossref |t Physical Review Letters |v 133 |y 2024 |x 0031-9007 |
| 773 | _ | _ | |a 10.1103/PhysRevLett.133.121401 |g Vol. 133, no. 12, p. 121401 |0 PERI:(DE-600)1472655-5 |n 12 |p 121401 |t Physical review letters |v 133 |y 2024 |x 0031-9007 |
| 787 | 0 | _ | |a Boskovic, Mateja et.al. |d 2024 |i IsParent |0 PUBDB-2024-00990 |r DESY-24-030 ; arXiv:2403.02415 |t Signatures of ultralight bosons in the orbital eccentricity of binary black holes |
| 856 | 4 | _ | |y OpenAccess |u https://bib-pubdb1.desy.de/record/616773/files/PhysRevLett.133.121401.pdf |
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