Jefferson Lab's New RWELL Detectors and Experiments
JLab is set to improve particle physics with innovative RWELL detectors.
Kondo Gnanvo, Florian Hauenstein, Sara Liyanaarachchi, Nilanga Liyanage, Huong Nguyen, Rafayel Paremuzyan, Stepan Stepanyan
― 6 min read
Table of Contents
- The Big Picture: High Luminosity Experiments
- Current Research Insights
- New Plans on the Table
- Enter the RWELL Detectors
- How Do RWELL Detectors Work?
- The Road Ahead: Testing the Prototypes
- The Setup: How Testing Works
- Early Results from the Tests
- The Big Prototype for CLAS12
- What the Large Prototype Looks Like
- The Learning Process: Efficiency Results
- The Impact of Dust
- Playing with Different Gases
- Looking Ahead
- Testing Continues
- A Team Effort
- Conclusion: A Bright Future
- Original Source
- Reference Links
Jefferson Lab (JLab) is getting ready to level up its experiments. They plan to use some fancy tools known as RWELL detectors to measure how particles behave when they collide. These new tools can handle a lot of activity at once, allowing scientists to gather more information than their current equipment allows. Basically, they want to see parts of particles (like quarks) and understand more about their structure, which is a bit like trying to see how a car is built from a distance.
The Big Picture: High Luminosity Experiments
High luminosity experiments are like hosting a party where everyone is invited, but some guests bring their entire family. It means lots of particles interacting at the same time. With these experiments, scientists can look for tiny reactions that are usually missed when things are less chaotic. JLab is looking to build bigger and better detectors to keep up with all this action.
Current Research Insights
So far, JLab has been working on experiments that give us glimpses into the world of quarks. They’ve already gathered some interesting data, but there’s still a lot more to find out. Some of the hidden secrets involve the internal workings of partons (the components of protons and neutrons). To uncover these mysteries, scientists want to study a process called Double Deeply Virtual Compton Scattering (DDVCS). It sounds complicated, but it’s just one of the ways to learn more about how particles interact.
New Plans on the Table
Recently, two proposals have been submitted to a group that advises JLab on experiments. These ideas involve using slightly modified versions of the CLAS12 detector and the SOLID detector in different areas of the lab. The goal is to run these experiments at a luminosity that’s even higher than what the CLAS12 detector normally operates at.
Enter the RWELL Detectors
RWELL detectors are a new type of technology designed to handle the high activity that comes from these experiments. They have a clever design that keeps things compact while using less material, which is great for keeping costs down. Just think of them as the sleek, high-tech gadgets in the particle world.
How Do RWELL Detectors Work?
The RWELL detectors are made up of two main parts: a cathode and a special kind of printed circuit board (PCB). The PCB has tiny holes (microwells) that amplify signals when particles pass through. They also have a resistive layer that prevents big discharges of electricity, which helps keep the detector stable. With less risk of sparks flying, these detectors can function better in busy environments.
The Road Ahead: Testing the Prototypes
At JLab, scientists are currently testing various RWELL prototypes to see how well they work in high-rate situations. These prototypes come in various sizes, with some designed for everyday use and others aimed specifically at high activity. The scientists are trying to figure out how different designs affect the detectors' performance.
The Setup: How Testing Works
For testing, JLab has set up a special area where scientists can check how the detectors perform when hit by Cosmic Particles. They’ve designed a flexible test stand that includes various tracking systems and sensors to monitor what happens when particles go through the detectors. Imagine it as a fancy lab bench where they can watch particle races!
Early Results from the Tests
Initial tests using cosmic rays show promise. The detectors are picking up signals as expected, and the results are pretty uniform across their surfaces. Despite some small issues caused by the grounding dots, the early signs indicate that they’re on the right track.
The Big Prototype for CLAS12
There’s also a larger RWELL prototype being tested for the CLAS12 project, a bit like the bigger brother of the regular detectors. This one has a trapezoid shape, making it the largest RWELL detector made so far. The goal is to see how well it does when it comes to detecting particles and handling noise.
What the Large Prototype Looks Like
The big prototype is layered with different types of strips that collect data. These strips run in two different directions, allowing the detector to measure hits from various angles. Picture it as a very efficient net catching all the information thrown at it!
The Learning Process: Efficiency Results
When the large prototype was tested with cosmic particles, scientists noticed several interesting patterns. For instance, certain areas had no activity, which was linked to some issues with high voltage in that part of the detector. It was as if some party guests had decided to sit out and not join the fun.
The Impact of Dust
There were also spots with low activity due to dust particles that got into the detector during adjustments. It's like when you throw a party and someone accidentally opens a window, letting in dust that messes with the fun. Despite these hiccups, it turns out that the detector can still work well, even with a bit of dust.
Playing with Different Gases
The scientists also tried out different gas mixtures to see how they affect efficiency. Two mixtures were tested: a common one and a second that is more stable. The results showed that the detector could operate at high Efficiencies with the second gas. It was like finding the right snack for the party – it kept everyone happy without causing chaos.
Looking Ahead
Even with a few challenges, the RWELL detectors are showing great potential. The hope is to build a new version of the large detector that will work even better. The plan involves creating two detectors that work together, which should enhance their performance.
Testing Continues
Moving forward, the next steps are to continue testing the smaller detectors for stability and efficiency under various conditions. They're planning to take these detectors into high-rate environments early next year, which will be like a grand test run in the real world.
A Team Effort
The success of these projects hinges on a lot of teamwork. Many individuals contribute their expertise, making sure everything runs smoothly from design to testing. It’s all hands on deck in the quest for particle knowledge!
Conclusion: A Bright Future
In summary, the RWELL detectors at Jefferson Lab are paving the way for exciting advancements in particle physics. With continued testing and development, scientists are optimistic about what they will uncover next. Who knows? They might just solve more of the universe's mysteries, one particle at a time!
In the realm of particle physics, every little bit of data is a treasure, and these RWELL detectors are on their way to becoming the treasure hunters we need. The journey may be filled with unexpected surprises, but that’s part of the adventure in science!
Title: uRWELL detector developments at Jefferson Lab for high luminosity experiments
Abstract: One of the future plans at Jefferson Lab is running electron scattering experiments with large acceptance detectors at luminosities $> 10^{37}cm^{-2}s^{-1}$. These experiments allow the measurements of the Double Deeply Virtual Compton Scattering (DDVCS) reaction, an important physics process in the formalism of Generalized Parton Distributions, which has never been measured because of its small cross-section. The luminosity upgrade of CLAS12 or the SOLID detector makes Jefferson Lab a unique place to measure DDVCS. One of the important components of these high luminosity detectors is a tracking system that can withstand high rates of $\approx 1MHz/cm^{2}$. The recently developed Micro-Resistive Well (uRWELL) detector technology is a promising option for such a tracking detector by combining good position resolutions, low material budget with simple mechanical construction, and low production costs. In this proceeding, we will discuss recent developments and studies with uRWELL detectors at Jefferson Lab for future upgrades of the CLAS12 detector to study the DDVCS reaction.
Authors: Kondo Gnanvo, Florian Hauenstein, Sara Liyanaarachchi, Nilanga Liyanage, Huong Nguyen, Rafayel Paremuzyan, Stepan Stepanyan
Last Update: 2024-11-27 00:00:00
Language: English
Source URL: https://arxiv.org/abs/2411.13734
Source PDF: https://arxiv.org/pdf/2411.13734
Licence: https://creativecommons.org/licenses/by/4.0/
Changes: This summary was created with assistance from AI and may have inaccuracies. For accurate information, please refer to the original source documents linked here.
Thank you to arxiv for use of its open access interoperability.
Reference Links
- https://orcid.org/#1
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- https://www.jlab.org/exp
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- https://www.jlab.org/Hall-B/ftof/manuals/FADC250UsersManual.pdf
- https://indico.cern.ch/event/1413681/contributions/6013367/attachments/2881828/5049134/The%20micro-RWELL%20for%20high-rate.pdf
- https://indico.cern.ch/event/1413681/contributions/6013367/attachments/2881828/5049134/
- https://wiki.jlab.org/physdivwiki/images/a/a9/CLAS12_high_lumi.pdf
- https://wiki.jlab.org/physdivwiki/images/a/a9/CLAS12
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- https://misportal.jlab.org/mis/physics/experiments/searchProposals.cfm