Add to ORKGThis talk will summarize the methods of testing and quality control that DRIFT IIe dark matter detectors underwent through the construction process. It will focus on the first series of steps to construct a detector; placing thousands of 50 \u27m diameter and 20 \u27m diameter wire 1 mm apart with minimal margin of error. I will discuss the physics behind why we require a spacing accuracy of less than a few percent. Additionally, I will explain how we measure the spacing between successive wires and calculate the margin of error, giving results from detectors constructed this summer and discussing these results
The calibration and performance of the Silicon Drift and Silicon Strip Detectors of the ALICE experi...
The series of upgrades to the Large Hadron Collider, culminating in the High Luminosity Large Hadron...
Having high spatial resolution and good energy response the silicon drift detector (SDD) finds speci...
I will be presenting a talk on the results of the DRIFT IIe Project for this summer. To begin I will...
After learning how to use the DipTrace circuit board design program, I was able to assist with three...
DRIFT (Directional Recoil Identification From Tracks) is a dark matter collaboration that uses Multi...
The LHC will explore physics at the energy frontier and will address many open questions in particle...
Dark Matter is one of the greatest mysteries in Physics today. DRIFT - a dark matter detector design...
In the MEG II detector, the measurement of the momentum of the charged particle is performed by a hi...
It is believed that about 90 to 99% of the mass of the universe is composed of a non-baryonic, non-l...
The CMS Collaboration plans to equip the very forward muon system with triple-GEM detectors that can...
This summer I worked on measuring the drift velocity and dispersion of ions in a miniature version o...
The biggest question in astrophysics and cosmology today is identifying the composition of the Unive...
The nature of dark matter, which comprises 85% of the matter density in the universe, is a major out...
More than 4000 silicon microstrip detector modules for the ATLAS semiconductor tracker will be produ...
The calibration and performance of the Silicon Drift and Silicon Strip Detectors of the ALICE experi...
The series of upgrades to the Large Hadron Collider, culminating in the High Luminosity Large Hadron...
Having high spatial resolution and good energy response the silicon drift detector (SDD) finds speci...
I will be presenting a talk on the results of the DRIFT IIe Project for this summer. To begin I will...
After learning how to use the DipTrace circuit board design program, I was able to assist with three...
DRIFT (Directional Recoil Identification From Tracks) is a dark matter collaboration that uses Multi...
The LHC will explore physics at the energy frontier and will address many open questions in particle...
Dark Matter is one of the greatest mysteries in Physics today. DRIFT - a dark matter detector design...
In the MEG II detector, the measurement of the momentum of the charged particle is performed by a hi...
It is believed that about 90 to 99% of the mass of the universe is composed of a non-baryonic, non-l...
The CMS Collaboration plans to equip the very forward muon system with triple-GEM detectors that can...
This summer I worked on measuring the drift velocity and dispersion of ions in a miniature version o...
The biggest question in astrophysics and cosmology today is identifying the composition of the Unive...
The nature of dark matter, which comprises 85% of the matter density in the universe, is a major out...
More than 4000 silicon microstrip detector modules for the ATLAS semiconductor tracker will be produ...
The calibration and performance of the Silicon Drift and Silicon Strip Detectors of the ALICE experi...
The series of upgrades to the Large Hadron Collider, culminating in the High Luminosity Large Hadron...
Having high spatial resolution and good energy response the silicon drift detector (SDD) finds speci...