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

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7 The Source Runs in CTF2<br />

7.4 Analysis <strong>of</strong> the Source Runs<br />

7.4.1 Event Selection<br />

To select the Po alpha decay events, which originated from the Rn source, the following<br />

cuts were applied:<br />

- they are detected by the second electronic group;<br />

- they have a coincidence time delay <strong>of</strong> 10 s-1ms;<br />

- they have a pulse height in the range Ô Õ Ô ( Ô Õ Ô for<br />

source no. 2);<br />

- the preceding group 1 event ( Bi) has a pulse height between 100 <strong>and</strong> 1200 pe (the<br />

lower energy threshold is set to reject accidental coincidences involving C events);<br />

- there is no muon flag on this event or the preceding group 1 event.<br />

With these cuts, the Po alphas <strong>and</strong> the preceding Bi betas can be tagged very efficiently<br />

with negligible background. Their energy spectra are shown in fig. 7.6. Fitting an exponential<br />

to the coincidence time distribution reproduces very well the decay time <strong>of</strong> Po,<br />

Ø × ÐÒ<br />

Ø <br />

¡ ×<br />

while the fit gives ¡ × (see fig. 7.6, lower plot).<br />

Background<br />

The two sources <strong>of</strong> potential background events are Bi- Po events in the bulk scintillator<br />

volume <strong>and</strong> accidental coincidences:<br />

- The background due to Rn present in the scintillator containment vessel can be estimated<br />

to be at about the same level as in the previous runs before the source insertion,<br />

counts per hour. Due to the fact that the scintillator inside the source vial was<br />

quenched <strong>and</strong> the energy <strong>of</strong> the Po alpha peak shifted towards lower energies, the<br />

actual background contribution is even smaller.<br />

- The accidental background can be estimated by applying the energy cuts mentioned<br />

above for the group 1 <strong>and</strong> group 2 events, but taking a coincidence time window shifted<br />

to much greater delay times (7010 - 8000 s). For run 797 this gives an accidental background<br />

rate <strong>of</strong> counts per hour.<br />

Compared to the source activity <strong>of</strong> 200 - 800 counts per hour (for source 1 <strong>and</strong> 2 respectively)<br />

both background contributions are negligible.<br />

104

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