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A Scintillating Xenon Bubble Chamber for Dark Matter WIMP (Weakly Interactive Massive Particle) Detection!

Home PosterBoard CIERA-REU PICO Group Memories

Greetings,

My name is Jason Parks and this summer working as an intern with the CIERA-REU alongside PICO here at Northwestern University was very exciting. I was able to be apart of a project that is designing a prototype for direct detection of dark matter called a scintillating xenon bubble chamber. This dark matter particle detector is designed to look for Dark Matter particles from the Milky Way dark matter halo, which we think are continually flying through us. My chief responsibility this summer was testing the temperature and pressure control systems for the scintillating xenon bubble chamber. This required maintaining a temperature of -100 degrees Celsius in liquid nitrogen cooled cryostat. We used a closed loop PID (Proportional Integral Derivative) control method along with an internal heater to keep the detector environment at the desired temperature, with the goals of reaching a desired set point quickly and maintaining a temperature stable to within 0.01 degrees Celsius. With the PID control loop we achieved a temperature stable to 0.003 digress Celsius and accurate to 0.09 degrees Celsius, meeting the requirements for efficient detection.

We were to establish a stable temperature at which the temperature of xenon could be maintained at the desired superheated level (-100 degrees Celsius), in order to establish an environment in which we could observe WIMP interactions occurring via bubble nucleation. Bubble nucleation occurs when a liquid is heated slightly beyond its boiling point without boiling hence the term superheated. Particle interactions in the superheated liquid provide the energy needed to form a nucleation site, producing vapor bubbles in the superheated liquid. For dark matter detection, the degree of superheat must be strictly regulated at a level where WIMP interactions can nucleate bubbles. This requires precise control of the temperature and pressure of the target fluid. We also began construction of a hydraulic panel for pressure control and built the electrical system governing both temperature and pressure control readout for the detector.

Note: Project is still underway!

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Scintillating Xenon Bubble Chamber

Jason Parks
Email: jasoneparks84 [at] gmail [dot] com
CIERA-REU Intern
Northwestern University

This material is based upon work supported by the National Science Foundation under Grant No. AST-1359462, a Research Experiences for Undergraduates (REU) grant awarded to CIERA at Northwestern University. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation.