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Status: Bibliographieeintrag

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Verfasst von:Fell, Shaun [VerfasserIn]   i
 Heisenberg, Lavinia [VerfasserIn]   i
 Veske, Doğa [VerfasserIn]   i
Titel:Detecting fundamental vector fields with LISA
Verf.angabe:Shaun Fell, Lavinia Heisenberg, and Doğa Veske
E-Jahr:2023
Jahr:11 October 2023
Umfang:23 S.
Illustrationen:Illustrationen
Fussnoten:Gesehen am 08.05.2024
Titel Quelle:Enthalten in: Physical review
Ort Quelle:Ridge, NY : American Physical Society, 2016
Jahr Quelle:2023
Band/Heft Quelle:108(2023), 8 vom: Okt., Artikel-ID 083010, Seite 1-23
ISSN Quelle:2470-0029
Abstract:The advent of gravitational wave astronomy has seen a huge influx of new predictions for potential discoveries of beyond the Standard Model fields. The coupling of all fundamental fields to gravity, together with its dominance on large scales, makes gravitational physics a rich laboratory to study fundamental physics. This holds especially true for the search for the elusive dark photon, a promising dark matter candidate. The dark photon is predicted to generate instabilities in a rotating black hole spacetime, birthing a macroscopic Bose-Einstein condensate. These condensates can especially form around super massive black holes, modifying the dynamical inspiralling process. This then opens another window to leverage future space-borne gravitational wave antennas to join the hunt for the elusive dark matter particle. This study builds a preliminary model for the gravitational waveform emitted by such a dressed extreme mass-ratio inspiral. Comparing these waveforms to the vacuum scenario allows projections to the potential constrainability on the dark photon mass by space-borne gravitational wave antennas. The superradiant instability of a massive vector field on a Kerr background is calculated and, under reasonable approximations, the backreaction on the orbit of an inspiralling solar mass-scale compact object due to the secular evolution of the resulting boson cloud is determined. The end result is the projection that the LISA mission should be able to constrain the dark photon mass using extreme mass ratio inspirals in the range [1.8×10−17,4.47×10−16] eV.
DOI:doi:10.1103/PhysRevD.108.083010
URL:Bitte beachten Sie: Dies ist ein Bibliographieeintrag. Ein Volltextzugriff für Mitglieder der Universität besteht hier nur, falls für die entsprechende Zeitschrift/den entsprechenden Sammelband ein Abonnement besteht oder es sich um einen OpenAccess-Titel handelt.

Volltext: https://doi.org/10.1103/PhysRevD.108.083010
 Volltext: https://link.aps.org/doi/10.1103/PhysRevD.108.083010
 DOI: https://doi.org/10.1103/PhysRevD.108.083010
Schlagwörter:(s)LISA <Astronomie>   i
Datenträger:Online-Ressource
Sprache:eng
K10plus-PPN:1888116226
Verknüpfungen:→ Zeitschrift

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