18–24 Jun 2017
UC Irvine, Irvine, CA, USA
US/Pacific timezone

Dark matter velocity spectroscopy

20 Jun 2017, 17:50
20m
Pacific Ballroom AB (UC Irvine, Irvine, CA, USA)

Pacific Ballroom AB

UC Irvine, Irvine, CA, USA

Working Group Sessions Astroparticle Physics and Cosmology Working Group Working Group: Astroparticle physics and cosmology

Speaker

Dr Ranjan Laha (KIPAC, Stanford University and SLAC)

Description

ark 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. We demonstrate this technique using existing telescopes.

Primary author

Dr Ranjan Laha (KIPAC, Stanford University and SLAC)

Presentation materials