Results 21 to 30 of about 1,393 (196)

The CRESST II Dark Matter Search

open access: yesJournal of Physics: Conference Series, 2012
Talk at DSU workshop, ITP Beijing, Oct. 2011.
Leo Stodolsky, Karoline Schaffner
exaly   +3 more sources

Commissioning run of the CRESST-II dark matter search [PDF]

open access: yesAstroparticle Physics, 2009
The CRESST cryogenic direct dark matter search at Gran Sasso, searching for WIMPs via nuclear recoil, has been upgraded to CRESST-II by several changes and improvements.We present the results of a commissioning run carried out in 2007. The basic element of CRESST-II is a detector module consisting of a large (~ 300 g) CaWO_4 crystal and a very ...
G Angloher, J Imber, P Huff
exaly   +3 more sources

Results of the CRESST commissioning run 2007

open access: yes, 2016
CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) is a low temperature experiment dedicated to the direct dark matter detection via nuclear recoil. It is located in Hall A of the Laboratori Nazionali del Gran Sasso, Italy. Scintillating CaWO4 crystals operated at a few mK are utilized as target forWIMPs (Weakly Interacting Massive ...
Angloher, G   +24 more
openaire   +2 more sources

Analysis and modelling for CRESST-II [PDF]

open access: yes, 2012
The dark matter search CRESST-II completed its most recent run, Run 32, in 2011. Compared to previous runs, the quantity of data taken in this run increased significantly. In this work, Oxrop, analysis software in use within the CRESST collaboration, is upgraded to analyse this new data.
Brown, Andrew
openaire   +2 more sources

Probing spin-dependent dark matter interactions with $$^6$$ 6 Li

open access: yesEuropean Physical Journal C: Particles and Fields, 2022
CRESST is one of the most prominent direct detection experiments for dark matter particles with sub-GeV/c $$^2$$ 2 mass. One of the advantages of the CRESST experiment is the possibility to include a large variety of nuclides in the target material used ...
G. Angloher   +57 more
doaj   +1 more source

Interactions in Massive Colliding Wind Binaries [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2012
There are observational difficulties determining dynamical masses of binary star components in the upper HR diagram both due to the scarcity of massive binary systems and spectral and photometric contamination produced by the strong wind outflows in ...
Michael F. Corcoran
doaj   +1 more source

Searches for Light Dark Matter with the CRESST-III Experiment [PDF]

open access: yes, 2020
Cryogenic Rare Event Search with Superconducting Thermometers (CRESST) is a long-standing direct dark matter detection experiment with cryogenic detectors located at the underground facility Laboratori Nazionali del Gran Sasso in Italy.
Jochum, J.   +105 more
core   +2 more sources

Recasting direct detection limits within micrOMEGAs and implication for non-standard dark matter scenarios

open access: yesEuropean Physical Journal C: Particles and Fields, 2021
Direct detection experiments obtain 90% upper limits on the elastic scattering cross sections of dark matter with nucleons assuming point-like interactions and standard astrophysical and cosmological parameters.
G. Bélanger, A. Mjallal, A. Pukhov
doaj   +1 more source

Surprising Decrease in the Martian He Bulge During PEDE‐2018 and Changes in Upper Atmospheric Circulation

open access: yesJournal of Geophysical Research: Planets, Volume 128, Issue 8, August 2023., 2023
Abstract Using the Neutral Gas and Ion Mass Spectrometer (NGIMS) on the Mars Atmosphere Volatile and Evolution spacecraft (MAVEN), we analyzed data from Mars Year (MY) 32, 34, and 35 to examine the He bulge during the northern winter solstice (Ls ∼ 180–240), specifically focusing on the effects from the planet encircling dust event (PEDE‐2018).
Meredith K. Elrod   +3 more
wiley   +1 more source

Direct detection of dark matter: Precision predictions in a simplified model framework

open access: yesEuropean Physical Journal C: Particles and Fields, 2021
We present a calculation of the next-to-leading order QCD corrections for the scattering of Dark Matter particles off nucleons in the framework of simplified models with s- and t-channel mediators. These results are matched to the Wilson coefficients and
Christoph Borschensky   +4 more
doaj   +1 more source

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