We have developed an unconventional Transition Radiation Detector (SiTRD) based on silicon strip detectors (SSDs) operating inside a magnetic field. In this way, the path of the radiating particle is deflected with respect to the transition radiation X-rays that convert in a detector region far away from the charged particle track. In this paper we will show the results of a beam test performed at low momenta, up to 5 GeV/c, with a reduced scale detector prototype. We have also implemented a full Monte Carlo simulation to design a SiTRD for an accelerator or a cosmic ray experiment at higher momenta, up to 100 GeV/c. We have simulated two different detector configurations and we have studied their performance. (c) 2006 Elsevier B.V. All rights reserved.
A silicon transition radiation detector for space and accelerator applications / Brigida, M; Favuzzi, Cecilia; Fusco, P; Gargano, F; Giglietto, Nicola; Giordano, F; Loparco, F; Marangelli, B; Mazziotta, Mn; Mirizzi, N; Raino, S; Spinelli, P.. - In: NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH. SECTION A, ACCELERATORS, SPECTROMETERS, DETECTORS AND ASSOCIATED EQUIPMENT. - ISSN 0168-9002. - 564:1(2006), pp. 115-125. [10.1016/j.nima.2006.03.034]
A silicon transition radiation detector for space and accelerator applications
FAVUZZI, Cecilia;GIGLIETTO, Nicola;
2006-01-01
Abstract
We have developed an unconventional Transition Radiation Detector (SiTRD) based on silicon strip detectors (SSDs) operating inside a magnetic field. In this way, the path of the radiating particle is deflected with respect to the transition radiation X-rays that convert in a detector region far away from the charged particle track. In this paper we will show the results of a beam test performed at low momenta, up to 5 GeV/c, with a reduced scale detector prototype. We have also implemented a full Monte Carlo simulation to design a SiTRD for an accelerator or a cosmic ray experiment at higher momenta, up to 100 GeV/c. We have simulated two different detector configurations and we have studied their performance. (c) 2006 Elsevier B.V. All rights reserved.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
