PocketGeiger Type 5
For just initially poking around among the circuits downloaded from the SparkFun site, clearly the board is over-produced spillover from the little white plastic goodie that plugs into a smartphone. We note the 2012 date. We have a little smile at the Japanese transposition of "R" and "L" that extends from the way they pronounce into the documents spelling. "Open corrector output" is exactly what you think it should be, if ever you encountered "lestaurant".
First the PocketGeiger-5
I note there is the SIG radiation detection pulse, and the NS noise detection pulse.
The explanation is there is output a positive HIGH pulse when "vibration noise" has been detected a NS signal is delivered.
Hmm.. It would seem that in addition to detecting radiation, the chip is somewhat
microphonic. I suppose most any crystals are by the piezoelectric effect. That is concerning because of the very high outputs possible, and the fact we are to have some gain on the end of it.
The text at the end gives the clue that the NS pulse is used to trigger a dump to ignore the last 200mS of whatever is going on at the SIG connection. Quoting..
"Pulse width differs depending on vibration pattern and regardless of pull-up resistance R.
Dispose measurement data for last e [sec] {e<200[msec]} when vibration noise has been detected".
The circuit
We were agreed that the circuit is not best for what we want, and I get it that you may be using anything handy for now while checking it out.
The LMC662 is a OK CMOS OP-Amp. The original circuit is asking a lot to have a follower with 66M feedback resistor. The actual feedback current would be tiny. For most practical purposes, the 66M is almost not there! All the bias current the CMOS ever needs for the (+) input comes from the divider chain. I think the 1pF feedback is to keep it stable.
The (-) input works from only those few electrons that can fight their way through 66Mohms, and of course whatever might come out of the diode.
The bias condition of the diode is not obvious, done via 100K to a little switch-mode supply. At this stage, I admit I don't quite understand the thing.
It follows with a gain stage G=100, then offered at standard voltage window comparators in LM393. These are set to flip when the signal goes below 2.68V (assuming the 9V is exact). and when it goes above 3.09V. If it goes low, U3A output is open collector, looking to be pulled up hard by something it is hopefully connected to down the audio jack. current limited by 470 ohms. If it goes high, then U3B yanks the output low. If it is somewhere in between, regardless of diode noise and other information, things are quiet. I note the 4.7nF directly on the output of U3B open collector. There is no excuse for this! Let us bury this circuit now!
But we are not doing that!
We go linear instead, to try and extract whatever was yanking those comparators. I don't yet understand all of your Teensy circuit. How P2 selects the gain, and indeed how the signal makes it to the output. My search for HDR-IDC-2-54-2X3P did not find a datasheet - only 7 results of unrelated gabble.
PIN diode performance
The X100-7 SMD data sheet is encouraging. It is operated reverse biased. Looking at the dark current, I would choose to operate it at very little reverse bias, instead of the tens of volts as in the PocketGeiger. We see the "Absorption Probability" vs "Gamma Energy" graph. The main part of the curve is what I would call X-Rays. The graph is about the
probability of absorption, which is not the same thing as "
pulse height" nor "
duration".
This diode could apparently detect Chromium (5.4KeV), Vanadium (4.95KeV). From the graph, even Calcium and Potassium have more than 80% probability of being absorbed. Even Aluminium has a 30% probability. These probabilities are just that, and would not be directly related to the pulse size, only to how often they occur - whenever they do. We don't really know how much a given energy from incoming photons, once absorbed, will contribute to diode current above the dark current (which will be noisy racket)! It may not be much. I suppose we could estimate it, but I would just go for showing it some metal.
First thoughts about the detection
The thing is, the energy from the photons are not showing their presence with the help of huge gain, such as we would have from a PMT, or a avalanche diode. Therefore, I think, one needs to operate with as little bias as possible, limited by the PIN capacitance getting large enough to soak up the signal. Perhaps about 6V, where the dark current is is only 2nA, and capacitance (ugh) as much as 100pF. If the detection circuit can
still get pushed around enough in the face of 150pF, then 4V bias gets you 1.5nA dark current.
From then on, it is about capturing that (current) pulse and applying the sort of gain one would get from a PMT or avalanche diode. The amplifier has to have a bonkers low noise figure, and a gain that I am thinking should be more than 100. Perhaps 100,000? I cannot know without knowing what actually happens with a MX-100. Avalanche diode gains are around 10E5, and PMT gains are like 1.7E6.
A crazy thought.
The capacitance curve is so steep, it makes me think that if one used the PIN diode as part of a RF oscillator, the frequency shift when a pulse arrives just might be useful. We get here to the parametric amplifier techniques that used varactor diodes, very popular for avoiding noise, and widely used for radio telescopes and satellite receivers. Now, with availability of pHEMT FETs , one does not go to the expense of them, but for extreme low noise, they are still ultimate!
Enough with the crazy thought!
Why a buffer?
Of course - to stiffen up a high impedance signal. Is it that? It's from a diode, with a whole 3nA
of dark current. A stage with a gain of 1 adds the noise of it's first semiconductor molecules bashing around, and then it gets increased by as much again when it reaches the gain stage, so worsening the S/N ratio without yet any gain. You get an admittedly lower impedance signal, delivering a stiff, low impedance pile of extra noise!
I am thinking that a very low noise high gain stage is needed at the beginning. Bias, offset, signal clamping, etc, can all be dealt with, but the basic grab at the little current in excess of the dark current needs to be done right at the beginning, and brought to safety.
So, if I am wrong about all this, you can bet that I will just build yours!