Gravitationally Focused Dark Matter Around Compact Stars

TL;DR

This paper explores how gravitational focusing by compact stars can locally enhance dark matter density, potentially increasing observable annihilation signals, especially when combined with magnetic field effects.

Contribution

It introduces a model of dark matter density enhancement near compact stars due to gravitational focusing, highlighting potential observational signatures.

Findings

Density profile falls off as inverse square-root of distance

Magnetic fields can amplify annihilation signals

Local enhancement may produce detectable gamma-ray signals

Abstract

If dark matter self-annihilates then it may produce an observable signal when its density is high. The details depend on the intrinsic properties of dark matter and how it clusters in space. For example, the density profile of some dark matter candidates may rise steeply enough toward the Galactic Center that self-annihilation produces detectable gamma-ray emission. Here, we discuss the possibility that an annihilation signal may arise near a compact object (e.g., neutron star or black hole) even when the density of dark matter in the neighborhood of the object is uniform. Gravitational focusing produces a local enhancement of density, with a profile that falls off approximately as the inverse square-root of distance from the compact star. While geometric dilution may overwhelm the annihilation signal from this local enhancement, magnetic fields tied to the compact object can increase the signal's contrast relative to the background.