A Search for the Dark Matter Annual Modulation in South Pole Ice
arXiv:1106.1156 · doi:10.1016/j.astropartphys.2012.03.003
Abstract
Astrophysical observations and cosmological data have led to the conclusion that nearly one quarter of the Universe consists of dark matter. Under certain assumptions, an observable signature of dark matter is the annual modulation of 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.
FERMILAB-PUB-11-251-AE
References in corpus (13)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- First results from DAMA/LIBRA and the combined results with DAMA/NaI
- New results from DAMA/LIBRA
- Dark Matter Results from 100 Live Days of XENON100 Data
- The DAMA/LIBRA apparatus
- Final results of the EDELWEISS-II WIMP search using a 4-kg array of cryogenic germanium detectors with interleaved electrodes
- Improved Limits on Spin-Dependent WIMP-Proton Interactions from a Two Liter CFI Bubble Chamber
- Muon simulation codes MUSIC and MUSUN for underground physics
- Interpreting the recent results on direct search for dark matter particles in terms of relic neutralino
- Channeling in direct dark matter detection I: channeling fraction in NaI (Tl) crystals
- Temperature behavior of NaI (Tl) scintillation detectors
- Limits on the spin-dependent WIMP-nucleon cross-sections from the first science run of the ZEPLIN-III experiment
- A testable conventional hypothesis for the DAMA-LIBRA annual modulation
Cited by in corpus (19)
- Annual Modulation of Dark Matter: A Review
- Mirror dark matter: Cosmology, galaxy structure and direct detection
- Dark Matter Evidence, Particle Physics Candidates and Detection Methods
- Direct dark matter detection: the next decade
- Snowmass CF1 Summary: WIMP Dark Matter Direct Detection
- First search for a dark matter annual modulation signal with NaI(Tl) in the Southern Hemisphere by DM-Ice17
- Dark-Matter Harmonics Beyond Annual Modulation
- First data from DM-Ice17
- Decoherence as a way to measure extremely soft collisions with dark matter
- Dark Matter: A Brief Review
- Analysis of the 40K contamination in NaI(Tl) crystals from different providers in the frame of the ANAIS project
- Measurement of Muon Annual Modulation and Muon-Induced Phosphorescence in NaI(Tl) Crystals with DM-Ice17
- Scintillating bolometers: a key for determining WIMP parameters
- Review of Indirect WIMP Search Experiments
- Saas-Fee Lecture Notes: Multi-messenger Astronomy and Dark Matter
- Current status and projected sensitivity of COSINE-100
- Probing light WIMPs with directional detection experiments
- Bayesian analysis of multiple direct detection experiments
- DM-Ice: Current Status and Future Prospects