Dark matter direct-detection experiments
TM Undagoitia, L Rauch - Journal of Physics G: Nuclear and …, 2015 - iopscience.iop.org
In recent decades, several detector technologies have been developed with the quest to
directly detect dark matter interactions and to test one of the most important unsolved …
directly detect dark matter interactions and to test one of the most important unsolved …
Dark matter candidates from particle physics and methods of detection
JL Feng - Annual Review of Astronomy and Astrophysics, 2010 - annualreviews.org
The identity of dark matter is a question of central importance in both astrophysics and
particle physics. In the past, the leading particle candidates were cold and collisionless, and …
particle physics. In the past, the leading particle candidates were cold and collisionless, and …
Dark matter search results from the PICO-60 bubble chamber
C Amole, M Ardid, DM Asner, D Baxter, E Behnke… - Physical Review D, 2016 - APS
New data are reported from the operation of the PICO-60 dark matter detector, a bubble
chamber filled with 36.8 kg of CF 3 I and located in the SNOLAB underground laboratory …
chamber filled with 36.8 kg of CF 3 I and located in the SNOLAB underground laboratory …
micrOMEGAs_3: A program for calculating dark matter observables
G Bélanger, F Boudjema, A Pukhov… - Computer Physics …, 2014 - Elsevier
Abstract micrOMEGAs is a code to compute dark matter observables in generic extensions
of the standard model. This new version of micrOMEGAs is a major update which includes a …
of the standard model. This new version of micrOMEGAs is a major update which includes a …
Axions and the strong problem
JE Kim, G Carosi - Reviews of Modern Physics, 2010 - APS
Current upper bounds on the neutron electric dipole moment constrain the physically
observable quantum chromodynamic (QCD) vacuum angle| θ¯|≲ 10− 11. Since QCD …
observable quantum chromodynamic (QCD) vacuum angle| θ¯|≲ 10− 11. Since QCD …
The Tevatron at the frontier of dark matter direct detection
Direct detection of dark matter (DM) requires an interaction of dark matter particles with
nucleons. The same interaction can lead to dark matter pair production at a hadron collider …
nucleons. The same interaction can lead to dark matter pair production at a hadron collider …
First dark matter search results from a 4-kg bubble chamber <?format ?>operated in a deep underground site
E Behnke, J Behnke, SJ Brice, D Broemmelsiek… - Physical Review D …, 2012 - APS
New data are reported from the operation of a 4.0-kg CF 3 I bubble chamber in the 6800-foot-
deep SNOLAB underground laboratory. The effectiveness of ultrasound analysis in …
deep SNOLAB underground laboratory. The effectiveness of ultrasound analysis in …
Compatibility of DAMA/LIBRA dark matter detection with other searches
Abstract The DAMA/NaI and DAMA/LIBRA annual modulation data, which may be
interpreted as a signal for the existence of weakly interacting dark matter (WIMPs) in our …
interpreted as a signal for the existence of weakly interacting dark matter (WIMPs) in our …
The XENON100 dark matter experiment
The XENON100 dark matter experiment uses liquid xenon (LXe) in a time projection
chamber (TPC) to search for xenon nuclear recoils resulting from the scattering of dark …
chamber (TPC) to search for xenon nuclear recoils resulting from the scattering of dark …
Final analysis and results of the phase II SIMPLE dark matter search
M Felizardo, TA Girard, T Morlat, AC Fernandes… - Physical Review Letters, 2012 - APS
We report the final results of the Phase II SIMPLE measurements, comprising two run stages
of 15 superheated droplet detectors each, with the second stage including an improved …
of 15 superheated droplet detectors each, with the second stage including an improved …