Author:
Putignano O.,Muraro A.,Cancelli S.,Giacomelli L.,Gorini G.,Grosso G.,Kushoro M.H.,Marcer G.,Nocente M.,Perelli Cippo E.,Rebai M.,Tardocchi M.,Croci G.
Abstract
Abstract
In this paper we present the design of a photon pre-amplifier based on a photo-cathode
coated Thick Gas Electron Multiplier (THGEM). Such device is crucial in application where a weak
light signal produced in a radiation detector must be amplified so that it can be carried to a
photo-detector by means of optical fibres. An example of a device where a light signal must be
amplified is a gamma-ray Cherenkov detector for fusion power measurements in magnetic confinement
devices. In such application the active part of the detector must be located very close the
plasma, typically in a harsh radiation environment where standard photodetectors cannot operate.
The photon pre-amplifier allows to increase the signal generated in the active part of the
detector so that it can be easily detected by the photodetector located outside the harsh
environment. We present the conceptual design of a THGEM based photon pre-amplifier supported by
Garfield++ simulations. The device working principle is the following: primary photons impinge on
the photo-cathode and extract electrons that are accelerated by the THGEM electric field. Upon
collisions with the accelerated electrons, the gas molecules in the pre-amplifier are brought to
excited states and de-excite emitting scintillation photons. Since each electron excites multiple
gas molecules, the scintillation photons outnumber the primary photons, leading to the
amplification. In addition, we present the first observation of measurements of Nitrogen gas
scintillation in a THGEM device. We devised an experimental setup consisting of a vacuum chamber
containing a THGEM and an alpha particle source. The vacuum chamber is filled with pure nitrogen
and is coupled to a photomultiplier tube via a view-port to detect the scintillation photons
generated in the THGEM. For sake of simplicity the electrons that induce the scintillation are
generated by the ionization track of an alpha particle rather than by the THGEM photo-cathode
coating. A good qualitative agreement between simulations and experiment has been found, however
no quantitative conclusions can be made due to the lack of N2 excitation cross sections in
the Garfield++ code.
Subject
Mathematical Physics,Instrumentation