High-Energy Neutron Backgrounds for Underground Dark Matter Experiments

Abstract

A B S T R A C TDirect dark matter detection experiments usually have excellent capability to distinguish nuclear recoils, expected interactions with Weakly Interacting Massive Particle (WIMP) dark matter, and electronic recoils, so that they can efficiently reject background events such as gamma-rays and charged particles. However, both WIMPs and neutrons can induce nuclear recoils. Neutrons are then the most crucial background for direct dark matter detection. It is important to understand and account for all sources of neutron backgrounds when claiming a discovery of dark matter detection or reporting limits on the WIMP-nucleon cross section. One type of neutron background that is not well understood is the cosmogenic neutrons from muons interacting with the underground cavern rock and materials surrounding a dark matter detector.The Neutron Multiplicity Meter (NMM) is a water Cherenkov detector capable of measuring the cosmogenic neutron flux at the Soudan Underground Laboratory, which has an overburden of 2090 meters water equivalent. The NMM consists of two 2.2-tonne gadolinium-doped water tanks situated atop a 20-tonne lead target. It detects a high-energy (>∼ 50 MeV) neutron via moderation and capture of the multiple secondary neutrons released when the former interacts in the lead target. The multiplicity of secondary neutrons for the high-energy neutron provides a benchmark for comparison to the current Monte Carlo predictions. Combining with the Monte Carlo simulation, the muon-induced high-energy neutron flux above 50 MeV is measured to be (1.3 ± 0.2) × 10 −9 cm −2 s −1 , in reasonable agreement with the model prediction. The measured multiplicity spectrum agrees well with that of Monte Carlo simulation for multiplicity below 10, but shows an excess of approximately a factor of three over Monte Carlo prediction for multiplicities ∼ 10 − 20.In an effort to reduce neutron backgrounds for the dark matter experiment SuperCDMS SNO-LAB, an active neutron veto was developed. It is estimated that the current design of the neutron veto with a 40 cm thick layer of boron-doped liquid scintillator can achieve a > 90% efficiency for tagging the single-scatter neutrons. In addition, a one-quarter scale prototype detector for neutron veto has been built and tested. H I G H -E N E R G Y N E U T R O N B A C K G R O U N D S F O R U N D E R G R O U N D D A R K M A T T E R E X P E R I M E N T S Y U C H E N B . S . , B E I J I N G I N S T I T U T E O F T E C H N O L O G Y , B E I J I N G , C H I N A ( 2 0 0 6 ) M . S . , B E I J I N G N O R M A L U N I V E R S I T Y , B E I J I N G , C H I N A ( 2 0 0 9 ) D I S S E R T A T I O N S U B M I T T E D I N P A R T I A L F U L F I L L M E N T O F T H E R E Q U I R E M E N T S F O R T H E D E G R E E O F D O C T O R O F P H I L O S O P H Y I N P H Y S I C S S Y R A C U S E U N I V E R S I T Y D E C E M B E Dark MatterThere is compelling evidence for the existence of dark matter from astronomical and cosmological observations. In this chater, I will briefly present modern cos...

Cryogenic Detector Development for SuperCDMS

“…Before presenting the results themselves, we describe the methods used to obtain them.Background SpectraRare event searches such as SuperCDMS SNOLAB are limited by various backgrounds due to the detector material, cryostat, and laboratory environment. As such, Super-CDMS has devoted a tremendous amount of effort to assaying and tracking all materials and their contaminants as well as performing extensive modelling and simulations in efforts to understand and reduce all such backgrounds as far as possible[121,217,250,251,252,253]. The fruit of this labor is now readily available within the collaboration via tools such as the "Background Explorer", which provides the current best estimates of experimental background rates in the SuperCDMS SNOLAB experiment.…”