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Development of a Liquid Scintillator and of Data ... - Borexino - Infn

Development of a Liquid Scintillator and of Data ... - Borexino - Infn

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4.3 The Reconstruction Program<br />

detector, the time delay introduced by scattering <strong>and</strong>/or absorption-reemission processes, <strong>and</strong><br />

the time jitter <strong>of</strong> the PMT. The probability density function for a single photoelectron Ø is<br />

derived from a Monte Carlo simulation <strong>of</strong> the detector <strong>and</strong> archived in a look-up table. For the<br />

CTF, it is shown in fig. 4.7.<br />

Multiple Hits<br />

In the CTF the data acquisition registers only the arrival time <strong>of</strong> the first photoelectron for<br />

each electronic channel while the total number <strong>of</strong> photoelectrons per channel arriving within<br />

a time window <strong>of</strong> a few hundred nano seconds is recorded with an ADC. In BOREXINO the<br />

arrival time <strong>of</strong> each photoelectron will be recorded, if they arrive with at least 140 ns distance.<br />

In BOREXINO the probability for multiple hits is greatly reduced compared to the CTF, as<br />

each PMT covers a smaller solid angle. In the CTF, for a 1 MeV event the average value is 3<br />

hits per PMT, while in BOREXINO it will be only 0.2 hits per PMT.<br />

The probability for PMT , that the first one out <strong>of</strong> Ò photoelectrons has been registered at the<br />

time Ø can be calculated to be<br />

Ô ØÒ Ò ¡ Ø ¡<br />

<br />

Ø <br />

Ò <br />

where Ø is derived from the measured time Ø in the following way:<br />

Ø Ìevent Ø emission Ø flight Øscatter ¦ Ø jitter<br />

Ìevent Ø min Ü Ý Þ Ø<br />

Ø Ìevent Ø min Ü Ý Þ Ø<br />

Ø Ø Ø Ø min Ü Ý Þ Ø Ø min Ü Ý Þ<br />

The Ø min Ü Ý Þ are archived in a large multidimensional look-up table for each grid point<br />

<strong>and</strong> PMT (they are derived from the Monte Carlo simulation, which was described in the last<br />

section).<br />

Noise Hits<br />

The problem <strong>of</strong> (white) noise hits, which occur uncorrelated with the scintillation event, is<br />

equivalent to a probability density constant in time. This is already solved by substituting<br />

Ø with the maximum probability Å Ø . More correctly one has to add to Ø<br />

<strong>and</strong> renormalize afterwards. In practice this is equivalent to an additional constant bias to<br />

ÐÓ ÄÆØ× ¡ ÐÓ , which thus only slightly affects the minimization process. For a noise<br />

rate <strong>of</strong> 1 kHz one gets ¡ Ò× .<br />

<br />

55

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