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Rayleigh Scattering in Rare-Gas Liquids (CAT#: STEM-ST-0002-YJL)

Introduction

Recent advances in particle/astrophysics have created the need for low-background, large-mass particle detectors capable of measuring very small energy depositions. A number of novel detectors have been proposed to meet the requirements of the search for dark matter in the laboratory, the measurement of the spectrum of p–p neutrinos from the Sun and the observation of neutrinoless double β decay. Many of the proposals involve the use of rare-gas liquids, as this class of materials offers several advantages as large-mass, low-background absorbers. Being inert cryogenic fluids, the liquefied rare gases can be purified to levels not easily achieved in other materials.




Principle

The scattering of waves by small impurities (compared to the wavelength) is known as Rayleigh scattering, named after the British physicist who in 1871 first described this phenomenon quantitatively. Rayleigh scattering is a universal mechanism applicable to several contexts, from light scattering (damping of signals in optical fibres) to sound waves in solids and quantum-mechanical wavefunctions of electrons in disordered solids. Mathematically, Rayleigh scattering predicts a mean free path of the wave that varies with wavelength λ, proportional to 1/λ4.

Applications

Rayleigh scattering is used to analyze the properties of the Earth's atmosphere and used in optical communication systems. It is is applicable to scattering of UV and visible radiation by air molecules, infra-red radiation by small aerosols, and microwave radiation by cloud and rain drops.

Procedure

1. Sample preparation
2. Measurement by scattering detection instrument
3. Data analysis

Materials

Rayleigh scattering measurement system