0000000000178983

AUTHOR

P. C. F. Di Stefano

showing 2 related works from this author

Fracture Processes Observed with A Cryogenic Detector

2006

In the early stages of running of the CRESST dark matter search using sapphire detectors at very low temperature, 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 the energy release in fracture has been directly and accurately measured on a microscopic event-by-event basis. The energy threshold corresponds to the breaking of only a few hundred covalent bonds, a sensitivity some orders of magnitude greater than that of previou…

Physics - Instrumentation and Detectorsmedia_common.quotation_subjectDark matterGeneral Physics and AstronomyFOS: Physical sciencesAstrophysics01 natural sciencesAsymmetryPower law010305 fluids & plasmasHigh Energy Physics - Experiment[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Time domain[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsmedia_commonPhysicsHurst exponent[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]AutocorrelationAstrophysics (astro-ph)Instrumentation and Detectors (physics.ins-det)Computational physicsExponential functionOrders of magnitude (time)
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Fracture processes studied in CRESST

2005

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 appropriat…

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)
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