Large NaI(Tl) crystals as high energy resolution spectrometers in high energy physics and in γ-ray astronomy

1975 ◽  
Vol 22 (1) ◽  
pp. 286-291 ◽  
Author(s):  
L. H. O'Neill ◽  
R. L. Ford ◽  
R. Hofstadter ◽  
E. B. Hughes ◽  
R. Kose ◽  
...  

In this chapter a comparison between various designs of micropattern detectors is given, describing their specific advantages and disadvantages, which finally determines the fields of their applications. It is shown that at low counting rates the maximum achievable gas gain is determined by the Raether limit, which is about 106-107 electrons, depending on the design. At high counting rates, the maximum achievable gain additionally drops due to the contribution of several other effects (e.g. avalanches overlapping in space and time). Typically, micropattern detectors have a position resolution of ~30 µm, energy resolution of ~ 20% FWHM for 6 keV X-rays, and a time resolutions of ~1 ns. Some advanced designs offer even better characteristics. The diversity of micropattern detectors makes them attractive for many applications. For example, in measurements requiring simultaneously excellent time and position resolutions, mutigap multistrip detectors can be used in high energy physics applications, and hole-type structures are advantageous for the detection of visible photons. In some commercial applications, where reliability and robustness are important, spark protected detectors with resistive electrodes could be useful.


1994 ◽  
Vol 348 ◽  
Author(s):  
I. Dafinei ◽  
E. Auffray ◽  
P. Lecoq ◽  
M. Schneegans

ABSTRACTThe very large volumes needed to build a crystal calorimeter for High Energy Physics experiments bring cost considerations at the front of the stage. A reasonable compromise between cost and performances must be reached. One possible solution is to look at very dense materials like PbWO4, which will reduce the detector volume, even if the relatively low light yield will impose some limitations to the energy resolution. A review of the different results obtained by the Crystal Clear collaboration will be given for this crystal, including spectroscopic data and radiation damage measurements.


1995 ◽  
Vol 163 ◽  
pp. 495-503 ◽  
Author(s):  
Vladimir V. Usov

The stellar winds flowing out of the components of WR+OB binaries can collide and shock waves are formed. Stellar wind collision, particle acceleration by the shocks and generation of X-ray, γ-ray, radio and IR emission in WR+OB binaries are discussed.


2008 ◽  
Vol 45 (3) ◽  
pp. 43-49
Author(s):  
M. Shorohov ◽  
F. Muktepavela ◽  
J. Maniks

Surface Processing of TlBr Crystals for X- and γ-ray DetectorsA procedure for surface processing of TlBr crystals to be applied as X-and ?-ray detectors has been developed, providing removal of a mechanically destroyed surface layer by deep chemical etching, allowing the surfaces of good topography and thus the detectors with high energy resolution and stability to be obtained in a repeatable way. The surface quality and structural changes in the near-surface layer are estimated by the optical microscopy and indentation hardness technique.


Author(s):  
Preeti Kumari ◽  
◽  
Kavita Lalwani ◽  
Ranjit Dalal ◽  
Ashutosh Bhardwaj ◽  
...  

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