Abstract

A black hole image contains a bright ring of photons that have closely circled the black hole on their way from the source to the detector. Here, we study the photon ring of a rotating black hole which is pierced by a global hyper-light axion-type cosmic string. We show that the coupling \U0001d719F overset{sim }{F} between the axion \U0001d719 and the photon can give rise to a unique polarimetric structure of the photon ring. The structure emerges due to an Aharonov-Bohm type effect that leads to a change of the polarization directions of linear polarized photons when they circle the black hole. For several parameter choices, we determine concrete polarization patterns in the ring. Measuring these patterns can provide us with a way of determining the value of the coefficient of the mixed anomaly between electromagnetism and the symmetry that gave rise to the cosmic string. Finally, we briefly review a possible formation mechanism of black holes that are pierced by cosmic strings and discuss under which conditions we can expect such objects to be present as supermassive black holes in the center of galaxies.

Highlights

  • Very large baseline interferometry allows us to test aspects of fundamental physics that affect the structure and properties of the photon ring in the regime close to a black hole

  • We show that the coupling φF Fbetween the axion φ and the photon can give rise to a unique polarimetric structure of the photon ring

  • The structure emerges due to an Aharonov-Bohm type effect that leads to a change of the polarization directions of linear polarized photons when they circle the black hole

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Summary

Black hole pierced by a cosmic string

We shall introduce the objects which we are going to study in this work. We shall review some aspects of global cosmic strings in a U(1) invariant model. We review one mechanism of how black holes can become pierced by such strings in. We point out the existence of theoretical solutions that describe such pierced black holes restricting to the case of a cosmic string that coincides with the rotation axis of the black hole. We discuss how the pierced black holes evolve in time and under what conditions we can expect black holes pierced by cosmic strings to appear in the center of galaxies at present time

Global cosmic strings
Black hole piercing
Null geodesics in Kerr spacetime and bound orbits
Light ring
Impact of the cosmic string on the photons
Polarimetric signatures of the photon ring
Photon polarization
Time-averaged signatures
Time dependent signatures
Conclusion and outlook
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