4.6 Article

Lifshitz scaling, ringing black holes, and superradiance

Journal

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/1475-7516/2021/05/005

Keywords

gravitational waves / theory; quantum black holes; quantum gravity phenomenology

Funding

  1. JSPS Overseas Research Fellowships
  2. Perimeter Institute for Theoretical Physics
  3. Japan Society for the Promotion of Science [17H02890, 17H06359]
  4. World Premier International Research Center Initiative, MEXT, Japan
  5. Government of Canada through the Department of Innovation, Science and Economic Development Canada
  6. Province of Ontario through the Ministry of Research, Innovation and Science

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This study investigates the ringdown waveform and reflectivity of a Lifshitz scalar field around a fixed Schwarzschild black hole, finding that Lifshitz waves scattered by the black hole exhibit superradiance due to Lorentz breaking terms leading to superluminal propagation. This can allow Lifshitz waves to carry additional positive energy to infinity while leaving negative energy inside the Killing horizon, similar to the Penrose process in Kerr spacetime. The study also observes the emergence of long-lived quasinormal modes and drastic modifications to the greybody factor of a microscopic black hole with Hawking temperature comparable to the Lifshitz energy scale.
We investigate the ringdown waveform and reflectivity of a Lifshitz scalar field around a fixed Schwarzschild black hole. The radial wave equation is modified due to the Lorentz breaking terms, which leads to a diversity of ringdown waveforms. Also, it turns out that Lifshitz waves scattered by the Schwarzschild black hole exhibit superradiance. The Lorentz breaking terms lead to superluminal propagation and high-frequency modes can enter and leave the interior of the Killing horizon where negativity of energy is not prohibited. This allows the Lifshitz waves to carry out additional positive energy to infinity while leaving negative energy inside the Killing horizon, similar to the Penrose process in the ergosphere of a Kerr spacetime. Another interesting phenomenon is emergence of long-lived quasinormal modes, associated with roton-type dispersion relations. These effects drastically modify the greybody factor of a microscopic black hole, whose Hawking temperature is comparable with or higher than the Lifshitz energy scale.

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