The Gravitational Memory of a Galaxy

TL;DR

This paper investigates whether gravitational memory effects from soft radiation could mimic dark matter in galaxy dynamics, concluding that the effect is negligible and not a viable alternative explanation.

Contribution

It introduces the concept of gravitational memory affecting galaxy observations and assesses its potential to explain dark matter phenomena, finding it insufficient.

Findings

The effect is too small to explain the Tully-Fisher relation.

The effect grows with universe age but is limited by cosmological horizons.

Classical linearized treatment is inadequate at large times.

Abstract

We argue that soft gravitational radiation leads to a misidentification of the angular momentum of stars seen in distant galaxies, and that this could be interpreted as an additional mass inside the orbit of the star. It is tempting to identify this with the modifications of Newtonian dynamics that have been claimed [1] to eliminate the necessity for dark matter. Simple estimates of the effect show that it is very small and does not have the right functional form to explain the Tully-Fisher relation. The effect does grow with the age of the universe, but if our universe is indeed dominated by a cosmological constant, then most galaxies will disappear beyond the cosmological horizon before the effect is observable. We conjecture that this effect can be thought of as a new kind of gravitational memory: a rotation of frames at infinity, relative to those near the galaxy. One of the conclusions of our work is that at very large times the linearized classical treatment of this problem is inadequate, and should be replaced by Weinberg's soft photon resummation. However, these times are so long that they do not appear relevant to the universe in which we live. Neither method of calculation leads to a significant effect on galaxy evolution.