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Violation in Mixing

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2.2 The BABAR detector. 69<br />

energies. The transverse size of the crystals is chosen to be comparable to the Molière radius achiev<strong>in</strong>g the<br />

required angular resolution at low energies while limit<strong>in</strong>g the total number of crystals and readout channels.<br />

The BABAR �� consists of a cyl<strong>in</strong>drical barrel and a conical forward end-cap: it had a full angle coverage<br />

<strong>in</strong> azimuth while <strong>in</strong> polar angle it extends from ��� Æ to � �� Æ correspond<strong>in</strong>g to a solid angle coverage<br />

of � <strong>in</strong> the CM frame. Radially the barrel is located outside the particle ID system and with<strong>in</strong> the<br />

magnet cryostat: the barrel has an <strong>in</strong>ner radius of � Ñ and an outer radius of ��� Ñ and it’s located<br />

asymmetrically about the <strong>in</strong>teraction po<strong>in</strong>t, extend<strong>in</strong>g �� Ñ <strong>in</strong> the backward direction and � � Ñ <strong>in</strong><br />

the forward direction. The barrel conta<strong>in</strong>s ��� crystals arranged <strong>in</strong> �� r<strong>in</strong>gs with identical crystals<br />

each: the end-cap holds � crystals arranged <strong>in</strong> eight r<strong>in</strong>gs, add<strong>in</strong>g up to a total of ��� crystals. They<br />

are truncated-pyramid CsI(Tl) crystals: they are tapered along their length with trapezoidal cross-sections<br />

with typical transverse dimensions of ��� ¢ ��� Ñ at the front face, flar<strong>in</strong>g out towards the back to about<br />

�� � Ñ . All crystals <strong>in</strong> the backward half of the barrel have a length of ��� Ñ: towards the forward<br />

end of the barrel, crystal lengths <strong>in</strong>crease up to �� Ñ <strong>in</strong> order to limit the effects of shower leakage from<br />

<strong>in</strong>creas<strong>in</strong>gly higher energy particles. All end-cap crystals are of �� Ñ length. The barrel and end-cap<br />

have total crystal volumes of �� Ñ and �� Ñ , respectively. The CsI(Tl) sc<strong>in</strong>tillation light spectrum has a<br />

peak emission at �� ÒÑ: two <strong>in</strong>dependent photodiodes view this sc<strong>in</strong>tillation light from each crystal. The<br />

readout package consists of two silicon PIN diodes, closely coupled to the crystal and to two low-noise,<br />

charge-sensitive preamplifiers, all enclosed <strong>in</strong> a metallic hous<strong>in</strong>g.<br />

A typical electromagnetic shower spreads over many adjacent crystals, form<strong>in</strong>g a cluster of energy deposit:<br />

pattern recognition algorithms have been developed to identify these clusters and to differentiate s<strong>in</strong>gle<br />

clusters with one energy maximum from merged clusters with more than one local energy maximum,<br />

referred to as bumps. The algorithms also determ<strong>in</strong>e whether a bump is generated by a charged or a<br />

neutral particle. Clusters are required to conta<strong>in</strong> at least one seed crystal with an energy above Å�Î:<br />

surround<strong>in</strong>g crystals are considered as part of the cluster if their energy exceeds a threshold of Å�Îor if<br />

they are contiguous neighbors of a crystal with at least Å�Îsignal. The level of these thresholds depends<br />

on the current level of electronic noise and beam-generated background.<br />

A bump is associated with a charged particle by project<strong>in</strong>g a track to the <strong>in</strong>ner face of the calorimeter: the<br />

distance between the track impact po<strong>in</strong>t and the bump centroid is calculated and if it is consistent with the<br />

angle and momentum of the track, the bump is associated with this charged particle. Otherwise it is assumed<br />

to orig<strong>in</strong>ate from a neutral particle.<br />

On average, ��� clusters are detected per hadronic event: � are not associated to any charged particle.<br />

Currently, the beam-<strong>in</strong>duced background contributes on average with �� neutral clusters with energy above<br />

Å�Î.<br />

At low energy, the energy resolution of the �� is measured directly with the radiative calibration source<br />

yield<strong>in</strong>g ���� ��� ¦ �� at �� Å�Î. At high energy, the resolution is derived from Bhabha scatter<strong>in</strong>g<br />

where the energy of the detected shower can be predicted from the polar angle of the electrons and positrons.<br />

The measured resolution is ���� � ��¦ � at ��� ��Î.<br />

The measurement of the angular resolution is based on the analysis of � and � decays to two photons of<br />

approximately equal energy: the resolution varies between about ÑÖ�� at low energy and ÑÖ�� at high<br />

energies.<br />

THE BABAR EXPERIMENT

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