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RESEARCH PRODUCT
Fracture processes studied in CRESST
Susan CooperFranz Von FeilitzschUrmas NagelLeo StodolskyL. ZerleF. PröbstJan ÅStrömW. SeidelY. A. RamachersC. BucciO. MeierP. C. F. Di StefanoJ. TimonenSergey UchaikinSergey UchaikinM. SistiH. KrausC. CozziniJ. Marchesesubject
PhysicsNuclear and High Energy Physics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]AutocorrelationDark matter01 natural sciencesPower law010305 fluids & plasmasComputational physicsNuclear physics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]81.05.-t; 05.40; 07.90.+c; 29.40.-v0103 physical sciencesFracture (geology)Time domain[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentationEvent (particle physics)Energy (signal processing)Noise (radio)description
In the early stages of running of the CRESST dark matter search with sapphire crystals as detectors, an unexpectedly high rate of signal pulses appeared. Their origin was finally traced to fracture events in the sapphire due to the very tight clamping of the detectors. During extensive runs the energy and time of each event was recorded, providing large data sets for such phenomena. We believe this is the first time that the energy release in fracture has been accurately measured on a microscopic event-by-event basis. The energy distributions appear to follow a power law, dN/dE proportional to E-beta, similar to the Gutenberg-Richter power law for earthquake magnitudes, and after appropriate translation, with a similar exponent. In the time domain, the autocorrelation function shows time correlations lasting for substantial parts of an hour. Some remarks are made concerning the possible role Of Such mechanical stress release processes in the noise of sensitive cryodetectors. (c) 2006 Elsevier B.V. All rights reserved.
year | journal | country | edition | language |
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2005-07-31 |