Add to ORKGAn overview of the application of Si(Li) detectors to cosmic-ray identification is presented. A vacancy-related defect in FZ silicon that can limit the lithium compensation process in Si(Li) detector fabrication is discussed and a gettering process to remove this defect is outlined. Computer simulation of the gettering process is shown to yield native point defect diffusivity and concentration values approaching those recently proposed by Gösele, Plöβl and Tan
Fabrication of the 100 mm diameter, 3 mm thick lithium-compensated silicon, Si(Li), detectors for th...
A model describing the passivation by Li atoms of acceptors arising from radiation damage in Si dete...
The response of Si-Si-CsI(Tl) and Si-CsI(Tl) telescopes with quality controlled detectors, developed...
An overview of the application of Si(Li) detectors to cosmic-ray identification is presented. A vac...
A silicon sensor with 64 large area pads (“pad” of 1 cm2 area) was developed to identify relativisti...
© 2019 IEEE. Large-area lithium-drifted silicon (Si(Li)) detectors, operable 150°C above liquid nitr...
Space-based and balloon-borne experiments, designed for direct measurements of the elemental composi...
The physics potential at future hadron colliders as LHC and its upgrades in energy and luminosity Su...
Silicon strip detectors are fast, cost-effective and have an excellent spatial resolution.They are w...
A silicon sensor with 64 large area pads ("pad" of 1 cm 2 area) was developed to identify relativis...
In current particle physics experiments, silicon strip detectors are widely used as part of the inne...
Currently, most cosmic ray data are obtained by detectors on satellites, aircraft, high-altitude bal...
In current particle physics experiments, silicon strip detectors are widely used as part of the inne...
High Energy Physics experiments at future very high luminosity colliders will require ultra radiatio...
In 2007, ACCESS (Advanced Cosmic ray Composition Experiment for the Space Station) on the Internatio...
Fabrication of the 100 mm diameter, 3 mm thick lithium-compensated silicon, Si(Li), detectors for th...
A model describing the passivation by Li atoms of acceptors arising from radiation damage in Si dete...
The response of Si-Si-CsI(Tl) and Si-CsI(Tl) telescopes with quality controlled detectors, developed...
An overview of the application of Si(Li) detectors to cosmic-ray identification is presented. A vac...
A silicon sensor with 64 large area pads (“pad” of 1 cm2 area) was developed to identify relativisti...
© 2019 IEEE. Large-area lithium-drifted silicon (Si(Li)) detectors, operable 150°C above liquid nitr...
Space-based and balloon-borne experiments, designed for direct measurements of the elemental composi...
The physics potential at future hadron colliders as LHC and its upgrades in energy and luminosity Su...
Silicon strip detectors are fast, cost-effective and have an excellent spatial resolution.They are w...
A silicon sensor with 64 large area pads ("pad" of 1 cm 2 area) was developed to identify relativis...
In current particle physics experiments, silicon strip detectors are widely used as part of the inne...
Currently, most cosmic ray data are obtained by detectors on satellites, aircraft, high-altitude bal...
In current particle physics experiments, silicon strip detectors are widely used as part of the inne...
High Energy Physics experiments at future very high luminosity colliders will require ultra radiatio...
In 2007, ACCESS (Advanced Cosmic ray Composition Experiment for the Space Station) on the Internatio...
Fabrication of the 100 mm diameter, 3 mm thick lithium-compensated silicon, Si(Li), detectors for th...
A model describing the passivation by Li atoms of acceptors arising from radiation damage in Si dete...
The response of Si-Si-CsI(Tl) and Si-CsI(Tl) telescopes with quality controlled detectors, developed...