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Probing Black Hole Magnetic Fields with QED

Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada
Author to whom correspondence should be addressed.
Galaxies 2018, 6(2), 57;
Received: 18 March 2018 / Revised: 11 May 2018 / Accepted: 20 May 2018 / Published: 24 May 2018
(This article belongs to the Special Issue The Bright Future of Astronomical X-ray Polarimetry)
The effect of vacuum birefringence is one of the first predictions of quantum electrodynamics (QED): the presence of a charged Dirac field makes the vacuum birefringent when threaded by magnetic fields. This effect, extremely weak for terrestrial magnetic fields, becomes important for highly magnetized astrophysical objects, such as accreting black holes. In the X-ray regime, the polarization of photons traveling in the magnetosphere of a black hole is not frozen at emission but is changed by the local magnetic field. We show that, for photons traveling along the plane of the disk, where the field is expected to be partially organized, this results in a depolarization of the X-ray radiation. Because the amount of depolarization depends on the strength of the magnetic field, this effect can provide a way to probe the magnetic field in black-hole accretion disks and to study the role of magnetic fields in astrophysical accretion in general. View Full-Text
Keywords: black holes; X-ray polarization; quantum electrodynamics; radiative corrections; magnetic field black holes; X-ray polarization; quantum electrodynamics; radiative corrections; magnetic field
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MDPI and ACS Style

Caiazzo, I.; Heyl, J. Probing Black Hole Magnetic Fields with QED. Galaxies 2018, 6, 57.

AMA Style

Caiazzo I, Heyl J. Probing Black Hole Magnetic Fields with QED. Galaxies. 2018; 6(2):57.

Chicago/Turabian Style

Caiazzo, Ilaria, and Jeremy Heyl. 2018. "Probing Black Hole Magnetic Fields with QED" Galaxies 6, no. 2: 57.

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