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The current inner silicon detectors at CDF (SVXIIa and L00) will not tolerate the radiation dose associated with high-luminosity running and will need to be replaced.
These observations are mapped according to limiting magnitude, a measure of luminosity that runs on a scale of zero to seven.
BESIII is a high precision, general purpose detector for the high luminosity e+e− collider, BEPCII, running at the tau-charm energy region.
The estimation is that the first barrel layer, located at 4.3 cm from the beam pipe, after 3 years of LHC running at full luminosity will become inefficient for position reconstruction.
The luminosity function depends on population type.
The stellar luminosity function is a description of the relative number of stars of different absolute luminosities.
This distribution of globular cluster luminosities is called the Globular Cluster Luminosity Function (GCLF).
The high-luminosity running of PEP-II through the end of the decade will increase the radiation level in the SVT above its design limit.
It is going to be inserted parasitically in SVT to study its capabilities to improve data taking during the high luminosity CDF runs.
The COT improves upon the tracking performance of the Run I CTC drift chamber (e.g., increased stereo capability) while at the same time successfully accommodating the smaller bunch crossing and higher luminosity of Run II.
As the expected luminosity for Run IIb at the Tevatron collider was initially envisioned to reach 15 fb−1, radiation tolerances of both devices were revisited, culminating in proposals for new systems.
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com