On the long-term evolution of razor-thin galactic discs: Balescu-Lenard prediction and perspectives

TL;DR

This paper demonstrates that the inhomogeneous Balescu-Lenard kinetic theory accurately predicts the long-term evolution of galactic razor-thin discs, highlighting the importance of collective effects, damping modes, and simulation softening.

Contribution

It provides a quantitative validation of kinetic theory predictions against simulations and offers new insights into collective effects and damping in disc evolution.

Findings

Kinetic theory captures average long-term disc evolution.

Collective effects significantly accelerate relaxation.

Damped modes influence orbital heating.

Abstract

In the last five decades, numerical simulations have provided invaluable insights into the evolution of galactic discs over cosmic times. As a complementary approach, developments in kinetic theory now also offer a theoretical framework to understand statistically their long-term evolution. The current state-of-the-art kinetic theory of isolated stellar systems is the inhomogeneous Balescu-Lenard equation. It can describe the long-term evolution of a self-gravitating razor-thin disc under the effect of resonant interactions between collectively amplified noise-driven fluctuations. In this work, confronting theoretical predictions to numerical simulations, we quantitatively show that kinetic theory indeed captures the average long-term evolution of cold stellar discs. Leveraging the versatility of kinetic methods, we then offer some new perspectives on this problem, namely (i) the crucial impact of collective effects in accelerating the relaxation; (ii) the role of (weakly) damped modes in shaping the disc's orbital heating; (iii) the bias introduced by gravitational softening on long timescales; (iv) the resurgence of strong stochasticity near marginal stability. These elements call for an appropriate choice of softening kernel when simulating the long-term evolution of razor thin discs and for an extension of kinetic theory beyond the average evolution. Notwithstanding, kinetic theory captures quantitatively the ensemble-averaged long-term response of such discs.