Detecting dark matter WIMPs in the Draco dwarf: A multiwavelength perspective

By Sergio Colafrancesco, S. Profumo, P. Ullio. 2006

135 citations recorded by the source corpus.

We explore the possible signatures of dark matter pair annihilations in the nearby dwarf spheroidal galaxy Draco. After investigating the mass models for Draco in the light of available observational data, we carefully model the dark matter density profile, taking advantage of numerical simulations of hierarchical structure formation. We then analyze the gamma-ray and electron/positron yield expected for weakly interacting dark matter particle (WIMP) models, including an accurate treatment of the propagation of the charged particle species. We show that unlike in larger dark matter structures—such as galaxy clusters—spatial diffusion plays here an important role. While Draco would appear as a pointlike gamma-ray source, synchrotron emission from electrons and positrons produced by WIMP annihilations features a spatially extended structure. Depending upon the cosmic ray propagation setup and the size of the magnetic fields, the search for a diffuse radio emission from Draco can be a more sensitive indirect dark matter search probe than gamma rays. Finally, we show that available data are consistent with the presence of a black hole at the center of Draco: if this is indeed the case, very significant enhancements of the rates for gamma rays and other emissions related to dark matter annihilations are expected.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/17086364c4ea8e703266363130112ed46d04b9cf

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

In Nuclear and High Energy Physics

Citations in the corpus

A COMPLETE SPECTROSCOPIC SURVEY OF THE MILKY WAY SATELLITE SEGUE 1: THE DARKEST GALAXY (2010, background): “…these same objects represent critical targets for indirect dark matter detection experiments (e.g., Baltz et al. 2000; Evans, Ferrer, & Sarkar 2004; Colafrancesco et al. 2007; Strigari et al. 2008b; Kuhlen, Diemand, & Madau 2008; Bringmann et al. 2009; Pieri et al. 2009; Martinez et al. 2009) and…”
The Dark Matter Annihilation Signal from Galactic Substructure: Predictions for GLAST (2008, background): “…based on four criteria: (i) a hadronic spectrum from monochromatic quarks, (ii) lack of time variability, (iii) spatial extent, and (iv) a lack of emission at shorter wavelengths, except for very diffuse inverse Compton and synchrotron radiation (Baltz & Wai 2004; Colafrancesco et al. 2006, 2007).”