Chris Hamilton Created 2026-10-24 Updated 2026-11-05
Chris Hamilton and Tobias Heinemann studied the collective gravitational response of a stellar system near a stability threshold. In their linear homogeneous model, transient Landau modes cancel the divergent contribution obtained by treating a perturbing mass's gravitational wake in isolation.[ref]
This connects mode dynamics with the interpretation of gravitational relaxation. A separately large contribution need not make the complete observable response large when coupled terms are retained consistently.
Tobias Heinemann Created 2026-10-24 Updated 2026-11-05
Tobias Heinemann and Chris Hamilton analysed how a stellar system responds to a moving perturbing mass. Their homogeneous-system calculation includes both the gravitational wake and collective Landau modes, whose apparent divergences cancel near marginal stability.[ref]
The result shows why retaining only the steady wake can misrepresent a slowly relaxing system. The assumptions about background distribution and the order of time and stability limits are part of the calculation.