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Cosmic Pixels

Re-creating an equivalent of a spark chamber to see trajectories of muons from cosmic rays

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My idea is that by combining small muon detectors, we might be able to see the trajectories of the particle showers caused by cosmic rays, similar to how a spark chamber works. To detect these muons, the common practice is to use a scintillating material and a very sensitive light sensor. There are now silicon versions of photomultipliers (SiPMs). The analog part can be simplified compared to the amplification stage needed for spectroscopy.


(Spark Chamber in CERN’s permanent exhibition “Microcosm”.)

Since the first time I saw the spark chamber at the CERN exhibition nearly 20 years ago, I’ve been fascinated by how particle trajectories are directly visible between the plates of these big tubes. This detector shows the paths of muons produced by cosmic rays in the upper atmosphere. It uses two large scintillators placed above and below the tubes, detecting two events happening simultaneously. When this occurs, it means a particle has crossed the detector, triggering high voltage between the plates and creating sparks along the ionized path of the particle.

Inspirations and idea

To detect these muons, the common practice is to use a scintillating material and a very sensitive light sensor. High-performance sensors, such as photomultiplier tubes, are very expensive and complicated to operate. However, there are now silicon versions of photomultipliers (SiPMs), which are at the heart of many projects involving scintillators for gamma-ray spectrometers or muon detectors. Below are some links to very interesting projects:

https://hackaday.io/project/185211-all-in-one-gamma-ray-spectrometer

https://hackaday.io/project/194457-pomelo-gamma-spectroscopy-module

http://cosmicpi.org/

My idea is that by combining small muon detectors, we might be able to see the trajectories of the particle showers caused by cosmic rays, similar to how a spark chamber works.

Scintillators

Luckily, I was able to get a piece of plastic scintillator, most likely made by Bicron. I discovered that cutting this material is rather delicate due to its low melting point. Any machining can melt the plastic. After trying different approaches, I got decent results with a large-teeth circular saw, rotating in water. To make the detector light-tight, I used aluminum foil and black tape.

I’m using the 3×3 mm BROADCOM AFBR-S4N44P014M SiPM. These are put in direct contact with the scintillator inside the wrapping.

SiPMs act like diodes: when placed in reverse with around 40 volts, a small amount of current creates a small voltage spike when a detection occurs. These voltage spikes are around a few millivolts and last a few nanoseconds.

Trigger

Microcontrollers cannot register such small and short signals directly. For the purpose of detecting a flash of light caused by a muon, the analog part can be simplified compared to the amplification stage needed for spectroscopy.

Using a high-speed op-amp (LMV793), I created a threshold detection that holds for a few microseconds, long enough to interrupt a small microcontroller.

Boards

To determine if a particle has crossed several scintillators, we need to propagate the detection status to surrounding detectors. If one detects a flash and one or more neighboring detectors also register something simultaneously, chances are high that a particle has crossed the detector.

Each board is connected to its neighbors, relaying the detection signal not only to the four directly adjacent units but also to the diagonal ones. This setup enables any matrix shape. Each pixel is autonomous but works with its close neighbors to assess coincidences. I chose the PIC16F18346 for flexibility; it is overkill for just controlling an SK6812 serial LED, but it offers options like using the DAC for threshold control.

First tests

Before buying many SiPMs, which cost around 20 euros each, I conducted a few tests to ensure the concept worked. I noticed some differences between boards, especially in threshold voltage. Therefore, my next iteration includes a potentiometer to adjust it.

Scaling up

Building more pixels and connecting them together highlighted how critical stable power supplies are. The 5-volt and 40-volt rails are propagated board-to-board via header connectors, and any imperfection could worsen as the matrix grows. Extra care must be taken to filter out any parasitic signals.

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  • Test with antiproton annihilation

    Muth6 days ago 0 comments

    I finally completed the 7×7 matrix, and looked for a way to test it. Are the trajectories drawn on the pixels really showing particle coming from the interaction of cosmic rays with earth atmosphere ?

    Luckily I could place the matrix close to the Extremely Low ENergy Antiproton synchrotron (ELENA), at Cern. The annihilation of antiproton produces pions that might be an artificial source similar to what happens with natural cosmic rays.

    Watch the video above and see how it works amazingly well. The pixels go crazy during the ELENA deceleration process as few antiprotons are lost on the vacuum pipe. And it is even more impressive when placed close to an extraction line.

    Conclusion so far

    I consider this hobby project as a draft, a proof of concept. But it seems reasonable to say we are tracing the trajectories of the shower of secondary particles created by cosmic rays, those high energy particles coming from space.

  • 6x6 matrix and trajectories

    Muth06/24/2024 at 14:06 0 comments

    After designing and printing a modular assembly to hold the cosmic pixels, I've reach 36 pixels in a 6x6 matrix. Below some picture of the assembly.

    And below some shots of nice particle traversal:

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Discussions

getz1953 wrote 5 days ago point

Really interested in this project but where do I get the details? For example, what are the dimensions of the scintillators?  How are vcc and ht generated? 

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mihai.cuciuc wrote 05/26/2024 at 23:38 point

wow, love it! I was thinking of making something similar with GM tubes but I think your solution is much more promising

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Muth wrote 05/27/2024 at 09:42 point

Thanks a lot !

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