Author:
Bressler M.,Lamb N.,Neilson R.,Windle S.
Abstract
Abstract
Understanding and quantifying the gamma-induced bubble
nucleation background in clean nuclear recoil detection bubble
chambers is of utmost importance to bubble chamber based dark matter
searches. We present data confirming the hypothesis that large Auger
cascades from high-Z elements such as iodine and xenon dramatically
increase the response of C3F8 bubble chambers
to gamma rays. These tests, performed with a small calibration
bubble chamber filled with
C3F8+𝒪(10) ppm xenon, show that the
probability of bubble nucleation scales with the rate of xenon
inner-shell vacancies, reaching values >10% per K-Shell vacancy
for Seitz thresholds of interest to future dark matter searches in
bubble chambers. We also place an upper limit on bubble nucleation
probability for argon Auger events, relevant to large future bubble
chambers which may contain some residual atmospheric argon after the
active fluid fill.
Subject
Mathematical Physics,Instrumentation