Ionization of Gravitational Atoms

APA

Stout, J. (2022). Ionization of Gravitational Atoms . Perimeter Institute for Theoretical Physics. https://pirsa.org/22020067

MLA

Stout, John. Ionization of Gravitational Atoms . Perimeter Institute for Theoretical Physics, Feb. 15, 2022, https://pirsa.org/22020067

BibTex

          @misc{ scivideos_PIRSA:22020067,
            doi = {10.48660/22020067},
            url = {https://pirsa.org/22020067},
            author = {Stout, John},
            keywords = {Particle Physics},
            language = {en},
            title = {Ionization of Gravitational Atoms },
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2022},
            month = {feb},
            note = {PIRSA:22020067 see, \url{https://scivideos.org/index.php/pirsa/22020067}}
          }
          

John Stout Harvard University

Source Repository PIRSA
Collection

Abstract

Superradiant instabilities may create clouds of ultralight bosons around black holes, forming so-called “gravitational atoms.” It was recently shown that the presence of a binary companion can induce resonant transitions between a cloud's bound states. When these transitions backreact on the binary's orbit, they lead to qualitatively distinct signatures in the gravitational waveform that can dominate the overall behavior of the inspiral. In this talk, I will show that the interaction with the companion can also trigger transitions from bound to unbound states of the cloud---a process which I will refer to as ``ionization,'' in analogy with the photoelectric effect in atomic physics. Here, too, there is a type of resonance with a similarly distinct signature, which may ultimately be used to detect any dark ultralight bosons that exist in our universe.

Zoom Link: https://pitp.zoom.us/j/97300299361?pwd=azhmVTR5VmpPQ1hwbkVHTUsrOGlJZz09