• Title of article

    Fracture processes studied in CRESST

  • Author/Authors

    إstrِm، نويسنده , , J. and Prِbst، نويسنده , , F. and Di Stefano، نويسنده , , P.C.F. and Stodolsky، نويسنده , , L. and Timonen، نويسنده , , J. A. Bucci، نويسنده , , C. and Cooper، نويسنده , , S. and Cozzini، نويسنده , , C. and Feilitzsch، نويسنده , , F.v. and Kraus، نويسنده , , H. and Marchese، نويسنده , , J. and Meier، نويسنده , , O. A. Nagel، نويسنده , , U. and Ramachers، نويسنده , , Y. and Seidel، نويسنده , , W. and Sisti، نويسنده , , M. ، نويسنده ,

  • Pages
    3
  • From page
    754
  • To page
    756
  • Abstract
    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, d N / d E ∝ E - β , 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.
  • Keywords
    Cryodetectors , Microfracture
  • Journal title
    Astroparticle Physics
  • Record number

    2028399