Results 171 to 180 of about 1,400 (197)

A stress-induced source of phonon bursts and quasiparticle poisoning. [PDF]

Nat Commun
Anthony-Petersen R, Biekert A, Bunker R, Chang CL, Chang YY, Chaplinsky L, Fascione E, Fink CW, Garcia-Sciveres M, Germond R, Guo W, Hertel SA, Hong Z, Kurinsky N, Li X, Lin J, Lisovenko M, Mahapatra R, Mayer A, McKinsey DN, Mehrotra S, Mirabolfathi N, Neblosky B, Page WA, Patel PK, Penning B, Pinckney HD, Platt M, Pyle M, Reed M, Romani RK, Santana Queiroz H, Sadoulet B, Serfass B, Smith R, Sorensen P, Suerfu B, Suzuki A, Underwood R, Velan V, Wang G, Wang Y, Watkins SL, Williams MR, Yefremenko V, Zhang J.   +45 more
europepmc   +1 more source

Stratified wind from a super-Eddington X-ray binary is slower than expected. [PDF]

Nature
XRISM collaboration.
europepmc   +1 more source

Multiple Probe Measurements at Uranus Motivated by Spatial Variability. [PDF]

Space Sci Rev
Wong MH, Rowe-Gurney N, Markham S, Sayanagi KM.   +3 more
europepmc   +1 more source

The CRESST Dark Matter Search [PDF]

Astroparticle Physics, 1999
We present first competitive results on WIMP dark matter using the phonon-light-detection technique. A particularly strong limit for WIMPs with coherent scattering results from selecting a region of the phonon-light plane corresponding to tungsten recoils.
Urmas Nagel, Monica Sisti, Sergey Uchaikin   +2 more
exaly   +17 more sources

The CRESST Dark Matter Experiment: Status and Perspectives

Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 2000
Abstract The CRESST experiment in its first phase is using sapphire detectors with tungsten phase transition thermometers to search for dark matter WIMPs. At present four 262 g detectors are performing first measurements under low background conditions. Detector performance as well as preliminary results from the background runs are presented.
Urmas Nagel, Daniele Pergolesi, Monica Sisti   +2 more
exaly   +3 more sources

First Results From the CRESST-III Low-Mass Dark Matter Program [PDF]

Physical Review D, 2019
The CRESST experiment is a direct dark matter search which aims to measure interactions of potential dark matter particles in an Earth-bound detector.
Elia Bertoldo, Lucia Canonica, Cenk Türkoğlu   +2 more
exaly   +3 more sources

Search for Dark Matter With CRESST

New Journal of Physics, 2009
Accepted for publication in New Journal of Physics.
Rafael Lang, Wolfgang Seidel
exaly   +3 more sources

Light Dark Matter in the Light of CRESST-II

Journal of Cosmology and Astroparticle Physics, 2012
Recently the CRESST collaboration has published the long anticipated results of their direct Dark Matter (DM) detection experiment with a CaWO_4 target. The number of observed events exceeds known backgrounds at more than 4 sigma significance, and this excess could potentially be due to DM scattering.
Thomas Schwetz, Jure Zupan, Joachim Kopp
exaly   +5 more sources

Toward a Consistent Picture for CRESST, CoGeNT, and DAMA

Physical Review D, 2012
11 pages, 7 ...
Dan Hooper
exaly   +4 more sources

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Detector calibration measurements in CRESST

Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 2006
Abstract The CRESST dark matter experiment uses the simultaneous measurement of the scintillation light and the heat signal of a CaWO 4 crystal to discriminate between background electron recoil and nuclear recoil events. At the Technical University of Munich calibration measurements have been performed to characterize the detectors.
W. Westphal, C. Coppi, F.v. Feilitzsch, C. Isaila, T. Jagemann, J. Jochum, J. König, T. Lachenmaier, J.-C. Lanfranchi, W. Potzel, W. Rau, M. Stark, D. Wernicke   +12 more
openaire   +1 more source