Violation in Mixing
Violation in Mixing
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