Authors

N. Belyaev, National Research Nuclear University MEPhI
M. L. Cherry, Louisiana State University
F. Dachs, European Organization for Nuclear Research
S. A. Doronin, National Research Nuclear University MEPhI
K. Filippov, National Research Nuclear University MEPhI
P. Fusco, Politecnico di Bari
F. Gargano, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
S. Konovalov, P.N. Lebedev Physical Institute of the Russian Academy of Sciences
F. Loparco, Politecnico di Bari
V. Mascagna, Istituto Nazionale di Fisica Nucleare, Sezione di Milano-Bicocca
M. N. Mazziotta, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
D. Ponomarenko, National Research Nuclear University MEPhI
M. Prest, Istituto Nazionale di Fisica Nucleare, Sezione di Milano-Bicocca
D. Pyatiizbyantseva, National Research Nuclear University MEPhI
C. Rembser, European Organization for Nuclear Research
A. Romaniouk, National Research Nuclear University MEPhI
A. A. Savchenko, National Research Nuclear University MEPhI
E. J. Schioppa, European Organization for Nuclear Research
D. Yu Sergeeva, National Research Nuclear University MEPhI
E. Shulga, National Research Nuclear University MEPhI
S. Smirnov, National Research Nuclear University MEPhI
Yu Smirnov, National Research Nuclear University MEPhI
M. Soldani, Istituto Nazionale di Fisica Nucleare, Sezione di Milano-Bicocca
P. Spinelli, Politecnico di Bari
M. Strikhanov, National Research Nuclear University MEPhI
P. Teterin, National Research Nuclear University MEPhI
V. Tikhomirov, National Research Nuclear University MEPhI
A. A. Tishchenko, National Research Nuclear University MEPhI
E. Vallazza, Istituto Nazionale di Fisica Nucleare, Sezione di Trieste
K. Vorobev, National Research Nuclear University MEPhI
K. Zhukov, P.N. Lebedev Physical Institute of the Russian Academy of Sciences

Document Type

Conference Proceeding

Publication Date

11-29-2019

Abstract

Many modern and future accelerator and cosmic ray experiments require identification of particles with Lorentz γ-factor up to 104 and above. The only technique which reaches this range of Lorentz factors is based on the transition radiation detectors (TRD). This paper describes the development of a TRD based on straw proportional tubes. A prototype of such kind of detector was built and tested at the CERN SPS accelerator. Monte Carlo simulation model of the detector which matches well the experimental data was developed. This program was used for the simulation of a full-scale TRD for hadron identification at TeV energy scale.

Publication Source (Journal or Book title)

Journal of Physics: Conference Series

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