6–9 Sept 2022
Physics Department, University "La Sapienza", Roma, Italy
Europe/Rome timezone

Photon-mediated dark-matter-nucleus interactions in the PICO-60 C3F8 bubble chamber

7 Sept 2022, 19:10
2m
corridor at the first floor, close to Aula Careri

corridor at the first floor, close to Aula Careri

Speaker

Alejandro Santiago García Viltres (Universidad Nacional Autónoma de México)

Description

The PICO-60 C3F8 dark matter detector was a bubble chamber consisting of a fused silica inner vessel filled with 52 kg of C3F8 in a superheated state operating at 2.45-keV and 3.29-keV thermodynamic thresholds, reaching exposures of 1404-kg-day and 1167-kg-day, respectively. This bubble chamber was operated two km deep underground at SNOLAB, in Sudbury, Ontario in Canada. These two searches established the most stringent direct-detection constraints to date on the WIMP-proton spin-dependent cross-section at 2.5×1041 cm2 for a 25 GeV/c2 WIMP. In this poster, the latest results from the PICO-60 detector will be presented, establishing coupling limits for photon-mediated dark matter-nucleus interactions using non-relativistic contact operators in an effective field theory framework.

Primary authors

Alejandro Santiago García Viltres (Universidad Nacional Autónoma de México) Eric Vazquez-Jauregui

Presentation materials