Thermal equilibrium of an ideal gas in a free-floating box
arXiv:2012.13273 · doi:10.1119/10.0004955
Abstract
The equilibrium and fluctuations of an ideal gas in a rigid container are studied by every student of statistical mechanics. Here we study the less well-known case when the box is floating freely; in particular we determine the fluctuations of the box in velocity and position due to interactions with the gas it contains. This system is a toy model for the fluctuations in velocity and position of a black hole surrounded by stars at the center of a galaxy. These fluctuations may be observable in nearby galaxies.
arXiv comment5 pages, no figures, submitted to American Journal of Physics
References in corpus (13)
- Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
- A geometric distance measurement to the Galactic Center black hole with 0.3% uncertainty
- An Eccentric Disk Model for the Nucleus of M31
- The Proper Motion of Sagittarius A*: III. The Case for a Supermassive Black Hole
- Evolution of Massive Black Hole Binaries
- Dynamics of a Massive Black Hole at the Center of a Dense Stellar System
- A Displaced Supermassive Black Hole in M87
- Henize 2-10: the ongoing formation of a nuclear star cluster around a massive black hole
- Brownian Motion of Black Holes in Dense Nuclei
- Direct N-body simulation of the Galactic centre
- Localizing Sagittarius A* and M87 on Microarcsecond Scales with Millimeter VLBI
- Brownian motion of supermassive black holes in galaxy cores
- Gravitational Brownian motion as inhomogeneous diffusion: black hole populations in globular clusters