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The results obtained in laboratory checks, using scintillator bars learn by silicon photomultipliers are reported. The current method is the first step for designing a precision monitoring system to be placed inside a free magnetized volume for everyday tracker tool the charge identification of low vitality crossing particles. The devised system is demonstrated able to offer a spatial resolution better than 2 mm. Scintillators, Photon Solid State detector, particle tracking gadgets. Among the many deliberate activities was the development of a mild spectrometer seated in a 20-30 m3 magnetized air volume, the Air Core Magnet (ACM). The entire design ought to be optimised for the willpower of the momentum and cost of muons within the 0.5 - 5 GeV/c range (the mis-identification is required to be less than 3% at 0.5 GeV/c). 1.5 mm is required contained in the magnetized air quantity. In this paper we report the outcomes obtained with a small array of triangular scintillator bars coupled to silicon photomultiplier (SiPM) with wavelength shifter (WLS) fibers.

This bar profile is here demonstrated in a position to offer the necessary spatial resolution in reconstructing the position of the crossing particle by profiting of the charge-sharing between adjoining bars readout in analog mode. SiPMs are wonderful candidates in changing standard photomultipliers in lots of experimental circumstances. Tests have been carried out with laser beam pulses and radioactive supply so as to characterize the scintillator bar response and SiPM behaviour. Here we briefly current the noticed behaviour of the SiPM used in our checks relating to the principle sources of noise and the effect of temperature on its response and linearity. Several models and packaging have been thought of. The principle source of noise which limits the SiPM’s single photon resolution is the "dark current" price. It's originated by cost carriers thermally created in the delicate volume and current in the conduction band and therefore it will depend on the temperature. The dependence of the dark present single pixel charge as a operate of the temperature has been investigated utilizing Peltier cells so as to alter and keep the temperature managed.

Dark current rate depends additionally on the Vwk as proven in Fig. 3. As a way to have low charges of dark current the value of Vbias has been fixed at 1.5 V giving a working voltage Vwk of 29 V. It is evident that, if obligatory, iTagPro shop it may be convenient to use a bias voltage regulator which automatically compensates for temperature variations. Not always the pixels of the SiPM work independently from one another. Photoelectrons (p.e.) can migrate from the hit pixel to another circuitously fired by a photon. Optical cross-speak between pixels results in a non-Poissonian behaviour of the distribution of fired pixels. An estimate of the optical cross talk probability will be obtained by the ratio double-to-single pulse charge as a perform of the temperature. The chance relies upon weakly on the temperature and ItagPro the measured degree of cross-talk (15-16%) is compatible with the one reported in the datasheet. SiPM response as soon as its primary parameters and cells configuration are given.

In the Fig. 4 it's shown the pulse peak distribution of the dark present for the SiPM below test. 0.2) mm diameter gap used to lodge a fiber to collect the sunshine. The lateral surface of the scintillator strips is painted with white EJ-510 TiO2 Eljen paint. The scintillation light is collected with 1.2 mm BCF-91A WaveLength Shifter (WLS) fiber produced by the Saint-Gobain Ltd. The WLS is glued into the opening operating along the bar and its ends are polished. The read-out is performed by the SiPM solely at one finish and the alternative side is mirrored with reflecting tape to maximize the sunshine collection. The entrance-finish board prototype devoted to the amplification and SiPM readout has been developed by the Bologna INFN digital group. The present from the SiPM is discharged on the low enter resistance of the transimpedance amplifier; this offers small time constants, that is, fast sign rise time (utilizing the OPA 656N with a 500 MHz bandwidth we obtain alerts with 20-30 ns of rise time).