[Submitted on 16 Jul 2015] (cross-list from astro-ph.CO)
Dark Matter Velocity Spectroscopy
Eric G. Speckhard🇺🇸 · Kenny C. Y. Ng🇺🇸 · John F. Beacom🇺🇸 · Ranjan Laha🇺🇸
Dark matter decays or annihilations that produce line-like spectra may be smoking-gun signals. However, even such distinctive signatures can be mimicked by astrophysical or instrumental causes. We show that velocity spectroscopy-the measurement of energy shifts induced by relative motion of source and observer-can separate these three causes with minimal theoretical uncertainties. The principal obstacle has been energy resolution, but upcoming experiments will reach the required 0.1% level. As an example, we show that the imminent Astro-H mission can use Milky Way observations to separate possible causes of the 3.5-keV line. We discuss other applications.
- Comments:
- 9 pages, 6 figures, supplemental materials and references added, minor numerical error fixed, conclusions unchanged
- Subjects:
- Cosmology and Nongalactic Astrophysics (astro-ph.CO); High Energy Astrophysical Phenomena (astro-ph.HE); High Energy Physics — Experiment (hep-ex); High Energy Physics — Phenomenology (hep-ph); Nuclear Theory (nucl-th)
- arXiv:
- 1507.04744 [pdf]