4.2 Article

A search for the dark matter annual modulation in South Pole ice

Journal

ASTROPARTICLE PHYSICS
Volume 35, Issue 11, Pages 749-754

Publisher

ELSEVIER
DOI: 10.1016/j.astropartphys.2012.03.003

Keywords

Dark matter; Direct detection; Annual modulation; DAMA; South Pole

Funding

  1. Wisconsin IceCube Particle Astrophysics Center
  2. Wisconsin Alumni Research Foundation
  3. Sloan Research Foundation
  4. National Science and Engineering Research Council of Canada
  5. University of Alberta
  6. Stewardship Science Graduate Fellowship
  7. Science Undergraduate Laboratory
  8. Fermilab
  9. United States Department of Energy [De-AC02-07CH11359]
  10. STFC [ST/K001337/1] Funding Source: UKRI
  11. Science and Technology Facilities Council [ST/K001337/1] Funding Source: researchfish

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Astrophysical observations and cosmological data have led to the conclusion that nearly one quarter of the Universe consists of dark matter. Should dark matter interact with nucleons, it has been postulated that an observable signature of dark matter is an annual modulation in the rate of dark matter-nucleon interactions taking place in an Earth-bound experiment. To search for this effect, we introduce the concept for a new dark matter experiment using NaI scintillation detectors deployed deep in the South Pole ice. This experiment complements dark matter search efforts in the Northern Hemisphere and will investigate the observed annual modulation in the DAMA/LIBRA and DAMA/NaI experiments. The unique location will permit the study of background effects correlated with seasonal variations and the surrounding environment. This paper describes the experimental concept and explores the sensitivity of a 250 kg NaI experiment at the South Pole. Published by Elsevier B.V.

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