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Universit`a degli studi Roma Tre Measurement of the KL meson ...

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28 CHAPTER 3. THE <strong>KL</strong>OE DETECTOR<br />

However, to calibrate <strong>the</strong> DC response and to monitor <strong>the</strong> 232 space-time relations<br />

<strong>the</strong>re is need for tracks with all possible orientations to simulate <strong>the</strong> <strong>KL</strong> decay<br />

products. This is done with cosmic rays. A calibration program, incorporated into<br />

<strong>the</strong> <strong>KL</strong>OE online system, automatically starts at <strong>the</strong> beginning <strong>of</strong> each run and<br />

selects about 80,000 cosmic-ray events. These events are tracked using <strong>the</strong> existing<br />

space-time relations and <strong>the</strong> average value <strong>of</strong> <strong>the</strong> residuals for hits in <strong>the</strong> central<br />

part <strong>of</strong> <strong>the</strong> cells is monitored. If <strong>the</strong> residuals exceed 40 µm <strong>the</strong>n about 300,000<br />

cosmic-ray events are collected and a new set <strong>of</strong> calibration constants is obtained.<br />

3.2 The Calorimeter<br />

The calorimeter [33] has been designed to satisfy a set <strong>of</strong> stringent requirements<br />

such as providing a hermetic detection <strong>of</strong> low energy photons with high efficiency,<br />

a reasonably good energy resolution and an excellent time and space resolution to<br />

reconstruct <strong>the</strong> vertex for <strong>the</strong> <strong>KL</strong> neutral decays. Then it is not only a calorimeter,<br />

but also a rough tracker and a time <strong>of</strong> flight detector. The calorimeter response has<br />

also to be fast since its signals are used to provide <strong>the</strong> main first-level trigger for <strong>the</strong><br />

events.<br />

The chosen solution for <strong>the</strong> EMC is a finely segmented sampling calorimeter,<br />

composed <strong>of</strong> lead passive layers and <strong>of</strong> scintillating fiber sensing layers. It is made<br />

<strong>of</strong> cladded 1 mm diameter scintillating fibers sandwiched between 0.5 mm thick lead<br />

foils. The foils are imprinted with grooves wide enough to accommodate <strong>the</strong> fibers<br />

and some epoxy, without compressing <strong>the</strong> fibers. This precaution prevents damage<br />

to <strong>the</strong> fiber-cladding interface. The epoxy around <strong>the</strong> fibers also provides structural<br />

strength and prevents light travelling in <strong>the</strong> cladding.<br />

About 200 such layers are stacked, glued, and pressed, resulting in a bulk material.<br />

The resulting composite has a fibers:lead:glue volume ratio <strong>of</strong> 48:42:10 which<br />

corresponds to a density <strong>of</strong> 5 g/cm 3 , an equivalent radiation length <strong>of</strong> X0 = 1.5<br />

cm and an electromagnetic sampling fraction <strong>of</strong> ∼13%. The large ratio <strong>of</strong> active<br />

material to radiator, <strong>the</strong> frequent signal sampling and <strong>the</strong> special fiber arrangement<br />

result in a factor √ 2 improvement in energy resolution with respect to calorimeter<br />

with slabs <strong>of</strong> equivalent scintillator to lead ratio.<br />

This material is shaped into modules 23 cm thick (∼15 X0). 24 modules <strong>of</strong><br />

trapezoidal cross section are arranged in azimuth to form <strong>the</strong> calorimeter barrel,<br />

aligned with <strong>the</strong> beams and surrounding <strong>the</strong> DC. An additional 32 modules with<br />

rectangular cross section, are wrapped around each <strong>of</strong> <strong>the</strong> pole pieces <strong>of</strong> <strong>the</strong> magnet<br />

yoke to form <strong>the</strong> endcaps, which hermetically close <strong>the</strong> calorimeter up to ∼98% <strong>of</strong><br />

4π, see Fig. 3.6. The unobstructed solid-angle coverage <strong>of</strong> <strong>the</strong> calorimeter as viewed<br />

from <strong>the</strong> origin is ∼94% [33].<br />

The fibers run parallel to <strong>the</strong> axis <strong>of</strong> <strong>the</strong> detector in <strong>the</strong> barrel, vertically in <strong>the</strong><br />

endcaps, and are connected at both ends to lucite light guides <strong>of</strong> area <strong>of</strong> 4.4×4.4<br />

cm 2 . The light guides are shaped as Winston cones with <strong>the</strong> o<strong>the</strong>r area coupled to<br />

<strong>the</strong> photocathode <strong>of</strong> fine mesh photomultipliers <strong>of</strong> 1.5 inches diameter with quantum<br />

efficiency <strong>of</strong> ∼20%. Thus each module is segmented in five consecutive layers<br />

each made <strong>of</strong> 4.4×4.4 cm 2 calorimeter cells. 4880 photomultiplier tubes view <strong>the</strong><br />

24+32+32 modules. The total length <strong>of</strong> scintillating fibers is 15,000 km.

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