PIRSA:19010062

Video URL

https://pirsa.org/19010062

Application of the black hole-fluid analogy: identification of a vortex flow through its characteristic waves

Weinfurtner, S. (2019). Application of the black hole-fluid analogy: identification of a vortex flow through its characteristic waves. Perimeter Institute for Theoretical Physics. https://pirsa.org/19010062

Weinfurtner, Silke. Application of the black hole-fluid analogy: identification of a vortex flow through its characteristic waves. Perimeter Institute for Theoretical Physics, Jan. 10, 2019, https://pirsa.org/19010062 

          @misc{ scivideos_PIRSA:19010062,
            doi = {10.48660/19010062},
            url = {https://pirsa.org/19010062},
            author = {Weinfurtner, Silke},
            keywords = {Quantum Gravity},
            language = {en},
            title = {Application of the black hole-fluid analogy: identification of a vortex flow through its characteristic waves},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2019},
            month = {jan},
            note = {PIRSA:19010062 see, \url{https://scivideos.org/index.php/pirsa/19010062}}
          }

Silke Weinfurtner University of Nottingham

Talk numberPIRSA:19010062
DOI10.48660/19010062
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

Black holes are like bells; once perturbed they will relax through the emission of characteristic waves. The frequency spectrum of these waves is independent of the initial perturbation and, hence, can be thought of as a `fingerprint' of the black hole. Since the 1970s scientists have considered the possibility of using these characteristic modes of oscillation to identify astrophysical black holes. With the recent detection of gravitational waves, this idea has started to turn into reality.
Inspired by the black hole-fluid analogy, we demonstrate the universality of the black-hole relaxation process through the observation of characteristic modes emitted by a hydrodynamical vortex flow. The characteristic frequency spectrum is measured and agrees with theoretical predictions obtained using techniques developed for astrophysical black holes. Our findings allow for the first identification of a hydrodynamical vortex flow through its characteristic waves.
The flow velocities inferred from the observed spectrum agree with a direct flow measurement. Our approach establishes a non-invasive method, applicable to vortex flows in fluids and superfluids alike, to identify the wave-current interactions and hence the effective field theories describing such systems.