z-logo
open-access-imgOpen Access
COUPP - a search for dark matter with a continuously sensitive bubble chamber
Author(s) -
Collar Juan,
K. Crum,
S. Mishra,
D. Nakazawa,
Brian Odom,
Julia Rasmussen,
Nathan Riley,
M. Szydagis,
E. Behnke,
Ilan Levine,
Nate Vander Werf,
P. S. Cooper,
M. Crisler,
Martin Hu,
E. Ramberg,
A. Sonnenschein,
R. Tschirhart
Publication year - 2007
Language(s) - English
Resource type - Reports
DOI - 10.2172/898400
Subject(s) - wimp , physics , bubble chamber , dark matter , detector , nuclear physics , weakly interacting massive particles , sensitivity (control systems) , particle physics , superheating , time projection chamber , minos , electron , optics , neutrino , astrophysics , engineering , neutrino oscillation , condensed matter physics , cosmology , electronic engineering , dark energy , scalar field dark matter
We propose to construct and operate a 60-kg room temperature CF{sub 3}I bubble chamber as a prototype dark matter (WIMP) detector. Operating in weakly-superheated mode, the chamber will be sensitive to WIMP induced nuclear recoils above 10 keV, while rejecting background electron recoils at a level approaching 10{sup 10}. We would first commission and operate this chamber in the MINOS near detector hall with the goal to demonstrate stable operation and measure internal contamination and any other backgrounds. This chamber, or an improved version, would then be relocated to an appropriate deep underground site such as the Soudan Mine. This detector will have unique sensitivity to spin-dependent WIMP-nucleon couplings, and even in this early stage of development will attain competitive sensitivity to spin-independent couplings

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom