Superfluid He4 is a promising target material for direct detection of light (<1 GeV) dark matter. Possible signal channels available for readout in this medium include prompt photons, triplet excimers, and roton and phonon quasiparticles. The relative yield of these signals has implications for the sensitivity and discrimination power of a superfluid He4 dark matter detector. Using a 16 cm3 volume of 1.75 K superfluid He4 read out by six immersed photomultiplier tubes, we measured the scintillation from electronic recoils ranging between 36.3 and 185 keVee, yielding a mean signal size of 1.25-0.03+0.03 phe/keVee, and nuclear recoils from 53.2 to 1090 keVnr. We compare the results of our relative scintillation yield measurements to an exi...
We investigate scintillation linearity of a commercial high pressure 4He gas detector using monoener...
The scintillation light yield of liquid argon from nuclear recoils relative to electronic recoils ha...
The PICO-500 bubble chamber will search for Weakly Interacting Massive Particles (WIMPs) at the SNOL...
Superfluid He4 is a promising target material for direct detection of light (<1 GeV) dark matter....
Superfluid $^4$He is a promising target material for direct detection of light ($<$ 1 GeV) dark matt...
A promising technology concept for sub-GeV dark matter detection is described, in which low-temperat...
We examine in depth a recent proposal to utilize superfluid helium for direct detection of sub-MeV m...
Abstract We explore the possibility of using superfluid helium for direct detection of sub-GeV dark ...
We have demonstrated in a pilot study using an existing experiment that superfluid He-3 at 100 mu K ...
This dissertation is an account of the first calorimetric detection of individual He*2 excimers with...
Using an existing experiment we have demonstrated in a pilot study that superfluid He-3 at 100 mu K ...
XENON10 is an experiment designed to directly detect particle dark matter. It is a dual phase (liqui...
The excitations in superfluid(3) He have a dispersion curve in which the energy minimum does not coi...
We show that a two-excitation process in superfluid helium, combined with sensitivity to meV energy ...
We show how a relativistic effective field theory for the superfluid phase of He4 can replace the st...
We investigate scintillation linearity of a commercial high pressure 4He gas detector using monoener...
The scintillation light yield of liquid argon from nuclear recoils relative to electronic recoils ha...
The PICO-500 bubble chamber will search for Weakly Interacting Massive Particles (WIMPs) at the SNOL...
Superfluid He4 is a promising target material for direct detection of light (<1 GeV) dark matter....
Superfluid $^4$He is a promising target material for direct detection of light ($<$ 1 GeV) dark matt...
A promising technology concept for sub-GeV dark matter detection is described, in which low-temperat...
We examine in depth a recent proposal to utilize superfluid helium for direct detection of sub-MeV m...
Abstract We explore the possibility of using superfluid helium for direct detection of sub-GeV dark ...
We have demonstrated in a pilot study using an existing experiment that superfluid He-3 at 100 mu K ...
This dissertation is an account of the first calorimetric detection of individual He*2 excimers with...
Using an existing experiment we have demonstrated in a pilot study that superfluid He-3 at 100 mu K ...
XENON10 is an experiment designed to directly detect particle dark matter. It is a dual phase (liqui...
The excitations in superfluid(3) He have a dispersion curve in which the energy minimum does not coi...
We show that a two-excitation process in superfluid helium, combined with sensitivity to meV energy ...
We show how a relativistic effective field theory for the superfluid phase of He4 can replace the st...
We investigate scintillation linearity of a commercial high pressure 4He gas detector using monoener...
The scintillation light yield of liquid argon from nuclear recoils relative to electronic recoils ha...
The PICO-500 bubble chamber will search for Weakly Interacting Massive Particles (WIMPs) at the SNOL...