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Title: Multi-Ton Argon and Xenon

Technical Report ·
DOI:https://doi.org/10.2172/993871· OSTI ID:993871

There is a wide range of astronomical evidence that the visible stars and gas in all galaxies, including our own, are immersed in a much larger cloud of non-luminous matter, typically an order of magnitude greater in total mass. The existence of this ''dark matter'' is consistent with evidence from large-scale galaxy surveys and microwave background measurements, indicating that the majority of matter in the universe is non-baryonic. The nature of this non-baryonic component is still totally unknown, and the resolution of the ''dark matter puzzle'' is of fundamental importance to cosmology, astrophysics, and elementary particle physics. A leading explanation, motivated by supersymmetry theory, is the existence of as yet undiscovered Weakly Interacting Massive Particles (WIMPs), formed in the early universe and subsequently clustered in association with normal matter. WIMPs could, in principle, be detected in terrestrial experiments by their collisions with ordinary nuclei, giving observable low energy (< 100 keV) nuclear recoils. The predicted low collision rates require ultra-low background detectors with large (0.1-10 ton) target masses, located in deep underground sites to eliminate neutron background from cosmic ray muons. The establishment of the Deep Underground Science and Engineering Laboratory for large-scale experiments of this type would strengthen the current leadership of US researchers in this and other particle astrophysics areas. We propose to detect nuclear recoils by scintillation and ionization in ton-scale liquid noble gas targets, using techniques already proven in experiments at the 0.01-0.1 ton level. The experimental challenge is to identify these events in the presence of background events from gammas, neutrons, and alphas.

Research Organization:
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE
DOE Contract Number:
AC02-07CH11359
OSTI ID:
993871
Report Number(s):
FERMILAB-PROPOSAL-1001; TRN: US1008192
Country of Publication:
United States
Language:
English