Noble Gas Detectors

169 citations recorded by the source corpus.

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

NEST: A Comprehensive Model for Scintillation Yield in Liquid Xenon (2011, methodology): “ep=N i. The deﬁnition ofW ef f i =W(1+a) is equivalent [4, 9, 41].6 Our model indicates that it should be 14.5 eV, in agreement with the 14.2 0.3 eV reported by Obodovskii and Pokachalov (as cited by [7]), but not with the oft-cited 15.6 0.3 eV ([9, 22] and ref. therein). The discrepancy is easily e”
Liquid noble gas detectors for low energy particle physics (2012, background): “s some recent advances and improvement attempts. The authors apologize in advance for inevitable incompleteness. More information can be found in other recently published monographs and review papers [5, 6, 7, 8, 9, 10]. The article is organized as follows. After motivating the search for particle d”
DARWIN dark matter WIMP search with noble liquids (2010, background): “2 The peak photon emission from the transition of exited dimers into their dissociative ground state is centered around 128 nm and 178 nm in liquid argon and xenon, respectively [25].”