29 March 2023 to 1 April 2023
UCLA
US/Pacific timezone

A Model-Independent Radio Telescope Search for Dark Matter in the S Band

30 Mar 2023, 11:00
15m
PAB- 1-425 (UCLA)

PAB- 1-425

UCLA

UCLA Department of Physics and Astronomy 475 Portola Plaza, Los Angeles, CA 90095

Speaker

Aya Keller

Description

Despite attempts to constrain the nature of dark matter over the last few decades, the parameter space has continuously broadened. We have designed a novel search technique for ultralight dark matter using the Breakthrough Listen public data release of Green Bank Telescope data that aims to match the broad theoretical scope with an equally broad model-independent strategy. The search concept depends only on the assumption of decay or annihilation of virialized dark matter to a quasi-monochromatic radio line, and additionally that the frequency and intensity of the line be consistent with most general properties expected of the phase space of our Milky Way halo. Specifically, the search selects for a line which exhibits a Doppler shift with position according to the solar motion through a static galactic halo, and similarly varies in intensity with position with respect to the galactic center [1]. After a development and testing stage performed on a narrow range in the L band, we have completed a full analysis of the S band.

We gratefully acknowledge support from the Heising-Simons Foundation under grants #2018-0989 and #2022-3566, and the Breakthrough Listen program.

  1. Aya Keller, et al., Astrophysics Journal 927, 71 (2022).

Primary authors

Presentation materials