Strong Gravity News & Events

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Correspondence of eikonal quasi-normal modes and unstable fundamental photon orbits for Kerr-Newman black hole

Speaker
Minyong Guo (Peking University, Beijing)
Event date
Venue
online (only)
Event type
In this work, we study the relation of the eikonal quasinormal modes (EQNMs) and the unstable fundamental photon orbits (UFPOs) in the Kerr-Newman spacetime. We find that in the eikonal limit the gravitational and electromagnetic perturbations of the Kerr-Newman black hole are naturally decoupled, and a single one-dimensional Schrodinger-like equation encoding the QNM spectrum can be derived.

Probing light axion-like particles with neutron star inspirals

Speaker
Jun Zhang (Imperial College, London)
Event date
Venue
online (only)
Event type
Despite of the weak couplings to normal matter, light axion fields can be significantly sourced by neutron stars, leaving potentially detectable signals in gravitational waves from binary neutron star inspirals. In this talk, I am going to talk about how the axions affect the inspiral waveform, and to report a recent search for such axions with GW170817.

Gravitational-wave imprints of non-integrable extreme-mass-ratio inspirals

Speaker
Kyriakos Destounis (University of Tübingen)
Event date
Venue
online (only)
Event type

Abstract: The detection of gravitational waves from extreme-mass-ratio inspirals (EMRIs) with upcoming space-borne detectors will allow for unprecedented tests of general relativity in the strong-field regime. Aside from assessing whether black holes are unequivocally described by the Kerr metric, they may place constraints on the degree of spacetime symmetry.

Black hole (de)scalarization in compact binaries

Speaker
Hector Silva (Max Planck Institute for Gravitational Physics)
Event date
Venue
online (only)
Event type
It was recently shown that a broad class of gravity theories allows for spontaneous scalarization of black holes, letting these objects grow “scalar hair” once certain conditions are met and to remain “bald” otherwise.

Quasinormal modes and their connection to black hole shadow

Speaker
Huan Yang (Perimeter Institute for Theoretical Physics)
Event date
Venue
online (only)
Event type

In this talk I will first review a few intriguing properties of black hole quasinormal modes in the eikonal limit or in the near extremal limit (for the black hole). After that I will show how to relate quasinormal modes to the black hole shadows, and how to formulate a test for such relation.

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