While traveling billions of lightyears, photons lose their energy. During my physics degree, the question of where that energy goes was never answered. I always thought it must be losing it to climbing in some gravitational potential, but which potential?? Sparked by a Veritasium video, I started pondering again. Maybe a part of its energy is lost to black-body radation?
Let's do a thought experiment. Imagine a (e.g. dust) particule in a spherical cavity of radius $R$, outside of which is a thermal bath, all in thermal equilibrium at constant temperature. If the cavity grows (slowly), the density of black-body radiation remains constant, and thus the particule's temperature as well. My reasoning is that even though the boundary of the cavity is further away, there is more of it that radiates into the cavity. Those cancel out exactly because had we started at a slightly larger radius, that would also be in thermal equilibrium. So when the radius grows to that size from a smaller radius to a bigger, we arrive in the state where it is still in equilibrium (assuming slow growth).
I would say our dust particule floating through space for billions of years does not enjoy this equilibrium. Imagine that $R$ is cosmological in scale, that the thermal bath is many many many galaxies, of the same temperature. When the galaxies recede, not more of them radiate to our particule (like our thermal bath's wall did). From our particule's perspective, a growing area of the sky darkens. Also less radiation from each galaxy hits the particule because of the nverse-square law. It's a crude model of cosmic expansion, but I hope it drives the point. Because the equilibrium is not maintained, I would conclude that our particule's temperature will decrease?
I chose a dust particule to delay dealing with the ill-defined temperature of a single fundamental particle, but let's consider a photon now instead:
- assuming that also a photon emits black-body radiation (here is a paper that seems to suggest so?)
- and assuming that if the photon emits more black-body radiation than it receives, it loses energy and thus redshifts
- and assuming that my simple model of receding distant galaxies sufficiently approximates cosmic expansion
Does a photon's redshift over the billions of years come from the cosmic expansion in part through this mechanism of black-body radiation being out of equilibrium?