Please use this identifier to cite or link to this item: http://hdl.handle.net/10773/18985
Title: Constraining black holes with light boson hair and boson stars using epicyclic frequencies and quasiperiodic oscillations
Author: Franchini, N.
Pani, P.
Maselli, A.
Gualtieri, L.
Herdeiro, C. A. R.
Radu, E.
Ferrari, V.
Issue Date: 2017
Publisher: American Physical Society
Abstract: Light bosonic fields are ubiquitous in extensions of the Standard Model. Even when minimally coupled to gravity, these fields might evade the assumptions of the black-hole no-hair theorems and give rise to spinning black holes which can be drastically different from the Kerr metric. Furthermore, they allow for self-gravitating compact solitons, known as (scalar or Proca) boson stars. The quasiperiodic oscillations (QPOs) observed in the x-ray flux emitted by accreting compact objects carry information about the strong-field region, thus providing a powerful tool to constrain deviations from Kerr's geometry and to search for exotic compact objects. By using the relativistic precession model as a proxy to interpret the QPOs in terms of geodesic frequencies, we investigate how the QPO frequencies could be used to test the no-hair theorem and the existence of light bosonic fields near accreting compact objects. We show that a detection of two QPO triplets with current sensitivity can already constrain these models and that the future eXTP mission or a LOFT-like mission can set very stringent constraints on black holes with bosonic hair and on (scalar or Proca) boson stars. The peculiar geodesic structure of compact scalar/Proca boson stars implies that these objects can easily be ruled out as alternative models for x-ray source GRO J1655-40.
Peer review: yes
URI: http://hdl.handle.net/10773/18985
DOI: 10.1103/PhysRevD.95.124025
ISSN: 2470-0010
Appears in Collections:CIDMA - Artigos
DFis - Artigos
GGDG - Artigos

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