English

DM-Ice: Current Status and Future Prospects

Instrumentation and Detectors 2019-08-14 v1 Cosmology and Nongalactic Astrophysics Instrumentation and Methods for Astrophysics High Energy Physics - Experiment

Abstract

DM-Ice is a program towards the first direct detection search for dark matter in the Southern Hemisphere with a 250 kg-scale NaI(Tl) crystal array. It will provide a definitive understanding of the modulation signal reported by DAMA by running an array at both Northern and Southern Hemisphere sites. A 17 kg predecessor, DM-Ice17, was deployed in December 2010 at a depth of 2457 m under the ice at the geographic South Pole and has concluded its 3.5 yr data run. An active R&D program is underway to investigate detectors with lower backgrounds and improved readout electronics; two crystals with 37 kg combined mass are currently operating at the Boulby Underground Laboratory. We report on the final analyses of the DM-Ice17 data and describe progress towards a 250 kg DM-Ice experiment.

Keywords

Cite

@article{arxiv.1510.00378,
  title  = {DM-Ice: Current Status and Future Prospects},
  author = {Walter C. Pettus},
  journal= {arXiv preprint arXiv:1510.00378},
  year   = {2019}
}

Comments

Talk presented CIPANP2015. 9 pages, 6 figures

R2 v1 2026-06-22T11:10:37.086Z