For a boosted strongly coupled plasma in d=2,3,4, holographic subregion complexity increases with temperature, velocity, and region size, and diverges as the Lorentz factor squared, gamma^2, when velocity approaches light speed.
Complexity of Scalar Collapse in Anti-de Sitter Spacetime
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We calculate the volume and action forms of holographic complexity for the gravitational collapse of scalar field matter in asymptotically anti-de Sitter spacetime, using numerical methods to reproduce the geometry responding to the oscillating field over multiple crossing times. Like the scalar field pulse, the volume complexity oscillates quasiperiodically before horizon formation. It also shows a scaling symmetry with the amplitude of the scalar field. The action complexity is also quasiperiodic with spikes of increasing amplitude.
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Holographic subregion complexity in a moving strongly coupled plasma
For a boosted strongly coupled plasma in d=2,3,4, holographic subregion complexity increases with temperature, velocity, and region size, and diverges as the Lorentz factor squared, gamma^2, when velocity approaches light speed.