A radiation sensor is a dispositive able to detect incoming ionizing particles (such us for example photons,β, gamma or or alfa particles) and gives to the user information like the energy, the intensity or the position of the radiation. Among the different approaches to the radiation detection, one of the most studied in the last decades is the usage of semiconductor solid state detector thanks to the continuous evolution of the semiconductor industries.
There are different families of detectors based on semiconductor substrates (Charge Coupled Devices CCD, Silicon Drift Detector SDD, PIN photodiode, etc. ) but the wide diffusion of the CMOS technologies in the consumer electronics has made very attractive all the implementations of such kind of technology in the field of radiation detectors; the growing diffusion of the CMOS imaging sensors is, for example, the most evident consequence of this fact.
All this page is focused on the most common implementation of a radiation sensor in CMOS technologies the Active Pixel Sensor.
The main element of this class of detectors is an inverse biased photodiode (see Figure 1 and Figure 2). When an incoming radiation with an energy near or greater than the silicon band gap crosses the depleted region of the p-n junction, some electrons can jump from the valence to the conduction band with the creation of electron hole pairs; the generated electron hole pairs are separated by the electric field of the junction and collected at the electrodes of the photodiode.
The generation of the electron-hole pairs is governed by the approximated relation: n = E / Ebg where n is the number of generated pairs, E is the energy released by the particle and Ebg is the band-gap energy of the silicon. In other words, the radiation generates a photo-current through the photodiode which can be measured directly or as a voltage drop at the ends of the junction. However, the photo-current discharges the photodiode reducing the depleted region and consequentially the sensibility of the detector; there are two techniques to avoid this phenomenon:
a) keep continuously the inverse polarization; in this case the voltage at the photodiode’s ends is always the same and, in order to detect the radiation, we have to measure the photo-current.
b) periodically recharge the photodiode by applying an inverse polarization for a given time and leaving the photodiode floating for the rest of the time. The voltage drop between the beginning and the end of the interval when the junction is left floating will be proportional to the integral of all the charge generated by the radiation during this time; due to this reason such time interval is usually named integration time.
This last approach is the most common in all the sensors arranged as a dense matrix of detectors because it requires less electronics near each photodiode.
In order to collect the maximum amount of the generated charge, the most common approach is to use a p-substrate where it is realized a small n-well, or a p++ substrate but with an epitaxial p-layer where it is realized the n-well (see Figure 1). In both ways the electrons will be collected by the n-well while the hole will be lost through the anode which is placed at the ground potential.
The benefit of this approach is that the mobility of the electrons is higher than the mobility of the holes and the charge collection is faster. The depleted region, in a conventional CMOS sensor, is very narrow due to the lower voltage for which this technology was originally developed; as consequence the charge does not reach the cathode for drift but rather for thermal diffusion. In this scenario it is fundamental the mean life of carriers in the p-layer. Such fact establishes a fundamental difference in the behaviour of the two different technological solutions: in case of epi-layer the sensitive thickness is limited by the thickness of the p-epi because in the p++ the carriers are affected by a faster recombination.
Figure 1 Two different technological implementations for the photodiode in CMOS technology, with (a), and without (b) epitaxial layer.
In Figure 2 (a) it is shown the conventional architecture of a three transistors APS. The photodiode is connected to the Vrst voltage through the transistor Mrst for the inverse polarization; turning off this transistor the photodiode is left floating. After a given integration time, turning on the Msel and imposing a constant current through the transistors Msf and Msel, the voltage at the cathode of the photodiode can be read at the pixel output.
Figure 2 (a) Electrical scheme of a standard three transistor APS, and (b) a simple 3x3 pixels matrix.
In a pixel sensor there are a big number of structures shown above, usually arranged in a rectangular matrix (in Figure 2 (b) there is an example of a 3x3 matrix). The reading of each pixel is performed row by row turning on all the Msel of the same row and imposing a current on each column line; at the end of each column can be read the voltage of the corresponding pixel of the selected row. The reset can be distributed row by row or common to all the pixels.
Figure 3 shows a typical output voltage of an APS pixel crossed by a β particle: during the reset interval the pixel is recharged to the reset voltage but, due to the parasitic capacitance between the gate and the source of Mrst, after this operation there is a little voltage drop. During the integration time, in dark condition, the voltage remains almost constant unless losses caused by the leakage current of the photodiode, but, if a particle or photon crosses the pixel, the generated charge causes a fast voltage drop. The signal of each pixel is in general measured as the difference between the initial value, at the beginning of the integration time, and the value at the end.
Figure 3 A typical output voltage of an APS crossed by a beta particle. The charge generated by the particle causes a clear voltage drop.
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